GEOLOGICA CARPATHICA, FEBRUARY 2005, 56, 1, 7790
Petrogenesis of convergent-margin calc-alkaline rocks and
the significance of the low oxygen isotope ratios: the Rodna-
Bârgãu Neogene subvolcanic area (Eastern Carpathians)
DELIA CRISTINA PAPP
1*
, IONEL URECHE
1
,
IOAN SEGHEDI
2
, HILARY DOWNES
3
and LUIGI DALLAI
4
1
Geological Institute of Romania, Cluj-Napoca Branch, P.O. Box 181, 400750 Cluj-Napoca, Romania; deliapapp@pcnet.ro
2
Institute of Geodynamics, Str. Jean-Luis Calderon 1921, 70201 Bucharest, Romania
3
Birkbeck/UCL Research School of Geological and Geophysical Sciences, Birkbeck College, Malet St., London WC1E 7HX,
United Kingdom
4**
Istituto di Geologia Ambientale e Geoingegneria IGAG, c/o Dipartimento Scienze della Terra, Università di Roma La Sapienza,
P.le Aldo Moro 5, 00185 Rome, Italy
**
Present address: CNRIstituto di Geoscienze e Georisorse, Area di Ricerca di Pisa, Via Moruzzi 1, 56127 Pisa, Italy
(Manuscript received March 28, 2003; accepted in revised form March 16, 2004)
Abstract: Neogene calc-alkaline magmatites (from basaltic andesites to rhyolites including mafic cognate enclaves) of
the Rodna-Bârgãu subvolcanic area (East Carpathian arc) are evaluated on the basis of new mineral compositional data,
major and trace elements, as well as Sr and O isotope data. Two different series of rocks have been separated. The
magmas of the medium-K series had a rapid ascent toward the surface, as proven by the presence of primary garnet
bearing rocks, or by the sporadic occurrence of mafic cognate enclaves. The δ
18
O values of amphiboles vary from 4.2 to
5.4 (SMOW). The δ
18
O value measured on garnet is 4.3 . The range of
87
Sr/
86
Sr ratios is from 0.70588 to 0.70887.
The decrease of the δ
18
O values as
87
Sr/
86
Sr ratios and SiO
2
increase is interpreted as a progressive contamination of a
mantle derived magma with a contaminant depleted in δ
18
O and enriched in
87
Sr/
86
Sr (i.e. hydrothermally altered lower
crustal rocks). Within the high-K series the presence of intermediate magma chambers where assimilation-fractional
crystallization processes took place is considered. The δ
18
O values measured on clinopyroxenes vary from 4.6 to 5.7
and on amphiboles from 3.8 to 6.7 . The range of
87
Sr/
86
Sr ratios is from 0.70605 to 0.70950. The covariation of the
δ
18
O values and
87
Sr/
86
Sr ratios is scattered. The highest δ
18
O values correspond to the highest
87
Sr/
86
Sr ratios and are
consistent with assimilation of the local upper-crustal rocks. The lower δ
18
O values and the observed oxygen isotope
disequilibrium between coexisting pyroxenes and amphiboles are explained by interaction with heated meteoric water.
Key words: Eastern Carpathians, subvolcanic intrusions, calc-alkaline magmas, crustal interaction, enclaves, low δ
18
O.
Introduction
Neogene magmatic rocks of the Inner Carpathian arc have
been the subject of many recent studies (e.g. Salters 1988;
Downes et al. 1995; Mason et al. 1996, 1998; Seghedi et al.
1995, 2001). However, there are as yet few published data on
the subvolcanic zone in the East Carpathian arc (e.g. Ureche et
al. 1995; Papp 1999; Niþoi et al. 2002). Here we report the first
detailed geochemical and isotopic study on Neogene magmat-
ic rocks from the Rodna-Bârgãu Mountains (Romania), which
form the main area of the subvolcanic zone. We evaluate the
calc-alkaline magmatism on the basis of new mineral compo-
sitional data, major and trace elements, as well as Sr and O
isotope data. The role of the mantle source, crustal assimila-
tion and magma mixing is addressed. Parental magmas show-
ing a depleted oxygen isotope signature relative to average
MORB are a special feature of the magmatic rocks from the
Rodna-Bârgãu Mountains. They are interpreted in terms of as-
similation of hydrothermally altered crustal rocks and interac-
tion between intrusive bodies and heated meteoric water.
Up to now, similar low δ
18
O rocks have not been reported
within the Carpathian Neogene volcanic arc. More extended
occurrences of rocks (e.g. alkaline basalts, granulite enclaves)
depleted in oxygen isotope have been described in the Pan-
nonian Basin (e.g. Kempton et al. 1997; Dobosi et al. 2003),
but those are related to the distensional efforts behind the Car-
pathian arc.
Worldwide, significantly
18
O-depleted primary magmas
have been recovered from plume derived basalts erupted in
ocean island settings (e.g. Iceland, Hawaii, Canary Islands)
(Eiler 2001 and literature therein). The origin of this low δ
18
O
signature has been attributed to either interaction of basaltic
magmas within the hydrothermally-altered lower oceanic crust
or as a primary feature of the plume itself. For the more
evolved magmas from Canary Islands, Thirlwall et al. (1997)
favour an interpretation that their
18
O-depleted character
might have been acquired during contamination by hydrother-
mally altered rocks in the current lithosphere.
Our study brings new arguments in the debate of the origin
of the
18
O-depleted magmas enforcing the importance of con-
www.geologicacarpathica.sk
*Corresponding author: E-mail: deliapapp@pcnet.ro; Tel./Fax:
+40264-429430
78 PAPP, URECHE, SEGHEDI, DOWNES and DALLAI
tamination by hydrothermally altered crustal rocks in conti-
nental arc-related magmatism. It also provides new data,
which might contribute to improving the models of geo-tec-
tonic evolution of the Inter-Carpathian area.
Geological setting of the Rodna-Bârgãu Mountains
Magmatic rocks in the Inner Carpathian arc are considered
by most authors (e.g. Csontos 1995; Balintoni 1996) to belong
to an active continental margin, connected to a subduction
zone located at the southwestern border of the Eurasian plate.
Although subduction was related to Alpine tectonic activity,
which started during the Cretaceous, the major convergent
event occurred in Miocene times (Sãndulescu 1984). Neogene
magmatism was associated with the consumption of a small
piece of ocean crust, attached to the European plate, beneath
the ALCAPA (Alpine-Carpathian-Pannonian) and Tisia-Getia
continental blocks (Rãdulescu & Sãndulescu 1976; Seghedi et
al. 1998).
The subvolcanic zone is located on the Tisia-Getia block
close to the boundary with both the ALCAPA block and the
Eastern European Plate, between the two volcanic segments:
Oaº-Gutâi in the north-west and Cãlimani-GurghiuHarghita
in the south-east (Fig. 1, insertion). Within the subvolcanic
zone numerous intrusive bodies are located in three areas:
Þibleº, Toroioaga and Rodna-Bârgãu.
In the Rodna-Bârgãu area special geological-structural con-
ditions resulted from the tectonic contact of the Rodna meta-
morphic massif with the Transcarpathian Flysch Zone, delin-
eated by the Someº Fault system (Fig. 1). The host-rocks of
the magmatites are crystalline schists of the Middle Dacides
and sedimentary deposits of the Transcarpathian flysch.
The intrusive bodies from the Rodna Mountains, hosted by
metamorphic rocks, are mostly large massive bodies (stocks,
and laccoliths associated with sills and dykes). More acidic fa-
cies are represented by: Parva rhyolites, Cormaia rhyodacites
and Valea Vinului quartz andesites (porphyritic micrograno-
diorites). In contrast, sedimentary flysch deposits form the
host-rocks of the intrusive bodies in the Bârgãu Mountains.
The main intrusive units are: Bucnitori and Sturzii (dacites),
Pleºii-Mal (quartz garnet andesites), Cornii (andesites),
Chicera and Arsente (Mãguri) (microdiorites) and Heniu,
Oala, Iliuþa, Colibiþa (South Bârgãu) (andesites). The intru-
sions vary in volume and have a surface exposure from 1 km
2
(Pleºii-Mal) to 20 km
2
(Cornii, Heniu).
Within the Rodna-Bârgãu area the age of the magmatites is
119 Ma, corresponding to Pannonian, similar to other volca-
nic activity in the Eastern Carpathians (Pécskay et al. 1995).
The distribution of ages among the delimitated intrusive units
is as follows: Sturzii 10.6±0.7 Ma, Runc 10.4±0.8 Ma, Valea
Vinului 9.0±0.5 Ma, Cornii 9.8±0.8 Ma, Mãgura Arsente
8.8±0.5 Ma, and Mãgura Rodnei 8.6±0.4 Ma.
Petrography of the magmatites
The main petrographic types of the Neogene magmatites are
basaltic andesites, microdiorites, quartz biotite amphibole
andesites, quartz-garnet andesites, dacites, rhyodacites, and
rhyolites. Transitional textures occur between subvolcanic and
plutonic facies, and between hypabyssal and volcanic-like fa-
cies. There is a relatively high degree of crystallization and
most of the rocks are porphyritic.
The main minerals are: plagioclase feldspars, amphiboles,
pyroxenes, biotite, quartz and subordinate potassic feldspars.
The accessory minerals are: apatite, magnetite, zircon, garnet
and the secondary minerals are: clay minerals, sericite, chlo-
rite, calcite, and epidote.
Magmatic cognate enclaves are relatively frequent in andes-
ites, microdiorites and diorites (Niþoi et al. 1995). They are
subangular to rounded in shape and vary from 23 cm up to
2025 cm in size. The cognate enclaves have a holocrystalline
hipidiomorphic structure, frequently showing a poikilitic char-
acter due to the presence of large amphibole crystals (mega-
crystals), which may include other minerals such as pyroxenes
and feldspars. The texture is massive. Amphiboles ± feldspars
represent the mineralogical composition of most cognate en-
claves, forming a hornblendite-like composition. Pyroxene ±
amphibole ± feldspars (pyroxenite-like) are also present.
Within the Valea Vinului quartz andesites, cog-
nate enclaves containing biotite + amphibole + feldspar oc-
cur. The contact between cognate enclaves and host-rocks is
either sharp or can show evidence of partial dissemination in
the host melt. Detailed petrographic descriptions of cognate
enclaves and their relationship with the host-rocks can be
found in Niþoi et al. (2002).
The magmas that generated the host-rocks in the Rodna-
Bârgãu Mountains had a calc-alkaline character and show a
complete differentiation trend, while the cognate enclaves are
much richer in FeO and MgO and display tholeiitic features
(Ureche 2000).
Sampling and analytical techniques
We have studied most of the important intrusive rocks in the
Rodna-Bârgãu sector. Samples of basaltic andesites, mi-
crodiorites, quartz biotite amphibole andesites, quartz garnet
andesites, dacites, rhyodacites and rhyolites, as well as mafic
cognate enclaves, were selected for whole rock and mineral
separates analysis.
For most of the whole-rock samples, major elements were
determined by wet chemical methods at the Prospecþiuni S.A.
(Bucharest) Laboratory. Trace elements and REE have been
determined by neutron activation method at the Geological In-
stitute of Romania. In addition, 23 pressed powder pellets
from the same whole-rock samples were made for determining
Rb, Sr, Y, Zr, Nb content by XRF analyses. For four samples
(I4/A2, I4/A3, I4px0, I4px4) complete chemical analysis (ma-
jor and trace elements) was performed by XRF. XRF analyses
have been carried out at the Department of Earth Science of
the La Sapienza University of Rome, using a PHILIPS 1480
Spectrometer equipped with a Rh tube running at 30 Kv
60 Ma for major elements and 50 Kv50 Ma for trace ele-
ments. Ba, La, Ce, Cr, and V have been performed by a W
tube running at 50 Kv50 Ma conditions. International stan-
dards were used for calibration and the precision and accuracy
PETROGENESIS OF CALC-ALKALINE ROCKS: NEOGENE SUBVOLCANIC AREA (EASTERN CARPATHIANS) 79
for major elements are estimated to be below 3 %. The analyt-
ical precision is better than 5 % for Rb, Sr and Y and better
than 10 % for other trace elements except for La and Ce,
which may be even more than 20 %.
The microprobe analyses were performed on polished thin
sections prepared within the laboratory of the CNR Centro
di Studio per il Quaternario e lEvolutione Ambientale, Rome
(at present Istituto di Geologia Ambientale e Geoingegneria).
The analyses were made using a CAMECA SX50 equipped
with 5 WDS spectrometers and one EDS Link eXL. Over 400
points distributed on profiles were measured on amphibole,
pyroxene, biotite, feldspar and garnet crystals.
Whole-rock powder samples of host rocks and cognate en-
claves were prepared for Sr isotope analyses. The isotope
analyses were carried out at the CNR Centro di Studio per
il Quaternario e lEvoluzione Ambientale, Rome. All samples
Fig. 1. Geological sketch map of the Rodna-Bârgãu Mountains. Intrusive magmatites (Pannonian): 1 rhyolites; 2 rhyo-dacites; 3
dacites; 4 quartz andesites ± biotite; 5 quartz garnet andesites; 6 andesites, a microdiorites, b diorites, c (hornblende ± py-
roxene); 7 basaltic andesites. Sedimentary cover: 8 shales, sandstones, pyroclastites (Lower Miocene); 9 sandstones (Borºa For-
mation) (Paleogene-Lower Miocene); 10 shales, standstones (Paleogene); 11 marls, shales, breccias (Priabonian-Paleogene); 12
limestones, sandstones, conglomerates (Lutetian-Priabonian). Metamorphic basement: 13 Rusaia metamorphic series (Silurian); 14
Rebra metamorphic series (Upper Proterozoic); 15 Bretila metamorphic series (Upper Proterozoic); 16 shear zone; 17 fault; 18
breccias; 19 pyroclastic products (Neogene).
80 PAPP, URECHE, SEGHEDI, DOWNES and DALLAI
were analysed in bulk, and the rocks were decomposed with a
mixture of ultrapure HF and HNO
3
in a teflon vessel at 70 °C
for 48 h. The resulting solution was evaporated and taken up
in 6.2 N ultrapure HCl. The Sr was separated in a 3 ml AG
50W-X8 resin column. Isotopic analyses were carried out us-
ing both Finnigan Mat 262RPQ multicollector and VG 54E
single collector mass spectrometers. For the latter machine,
the procedures of Ludwig (1994) were applied for data acqui-
sition and reduction. Internal precision (within-run precision)
of a single analytical result is given as two standard error of
the mean. Repeated analyses of standard NBS987 gave aver-
ages and errors expressed as 2 standard deviation as follows
87
Sr/
86
Sr=0.71024 +/2 (n=20) and the isotope ratios were
normalized to
86
Sr/
88
Sr to 0.1194.
Mineral separates of amphibole, pyroxene and garnet have
been analysed for O isotope ratios. Mineral separates were
made by hand picking under a microscope. In some cases sup-
plementary purification of the separates was performed, by
washing in an ultrasonic bath and/or acetone. Oxygen isotope
analyses were carried out at the CNR Centro di Studio per
il Quaternario e lEvolutione Ambientale, Rome, using a laser
fluorination system attached to a Finnigan MAT DELTA
plus mass spectrometer. Some samples have been replicated
or newly performed at the Royal Holloway University of Lon-
don using a laser fluorination system following the method de-
Table 1: Representative microprobe analyses of amphiboles of host rocks and enclaves. Abbreviations: Hen Heniu; V.Vin V.Vinului;
Chi Chicera; Ars Arsente; ro rock; en enclave; r rim; c core; pt potassian; tsch tschermakite; mghas mag-
nesiohastingsite; parg pargasite.
scribed by Mattey & Macpherson (1993). The determinations
made in Italy and the UK are comparable. Two or more ex-
tractions were made on each sample; the average reproducibil-
ity of isotopic analyses is ±0.2 or better. The analytical data
are reported in the δ-notation referenced to SMOW as the
mean of two or more replicate analyses.
Results
Main mineral species
Amphiboles are the main mafic minerals within the magmat-
ic rocks in the Rodna-Bârgãu area. All are Ca- rich and have
been classified according to IMA (Leake et al. 1997) nomen-
clature (Table 1). The magnesium number [Mg#=MgO/
(MgO+FeO)] varies from 0.53 (Valea Vinului cognate en-
clave) up to 0.87 (amphibole megacrystalArsente cognate en-
clave). Most amphibole phenocrysts, especially those found in
andesites and microdiorites are magnesiohastingsites. Am-
phiboles from more acidic facies are tschermakites. Amphib-
oles in cognate enclaves are also relatively heterogeneous, dis-
playing magnesiohastingsite (ChiceraArsente), pargasite
(Cornii) and tschermakite (Heniu) compositions. Zoning is
present within most of the amphibole crystals, both in host-
Sample
Anls.
Loc.
I15
ro(r)
Sturzii
I15
ro(c)
Sturzii
I31
ro
Pleºii
I8
ro
Hen
I8
en
Hen
I18
ro
Iliuþa
I11
ro
V.Vin
I11
ro
V.Vin
I5
ro
Chi
I5
en
Chi
I4
ro
Ars
I4
en(r)
Ars
I4
en(c)
Ars
I4mega
en
Ars
I14
ro
Cornii
I14
en
Cornii
SiO
2
44.53
41.98 41.90 43.06 42.72 43.37
40.95
40.72
42.44
42.70
42.08
41.52
42.64
42.73
42.95 43.27
TiO
2
0.91
1.00
0.69
1.05
1.86
2.18
1.47
1.83
1.30
1.21
1.67
1.87
1.46
1.19
1.95
2.15
Al
2
O
3
11.48
13.98 13.40 11.74 12.18 12.49
12.02
12.69
13.18
13.04
13.13
12.98
13.27
13.12
12.25 11.70
Cr
2
O
3
0.00
0.05
0.07
0.03
0.06
0.00
0.08
0.04
0.06
0.06
0.09
0.10
0.08
0.00
0.00
0.10
FeO*
15.96
16.82 17.99 17.51 13.83 14.32
18.69
16.25
9.54
8.86
11.52
13.51
9.52
10.56
12.11 11.50
MnO
0.62
0.51
0.51
0.60
0.23
0.25
0.56
0.35
0.10
0.16
0.23
0.32
0.15
0.15
0.28
0.20
MgO
12.18
10.50 10.33 11.37 12.61 12.75
9.25
10.69
15.28
15.79
14.13
12.68
15.58
15.16
12.77 13.85
CaO
9.78
10.37
9.88
9.56 11.12 10.19
11.35
11.21
11.68
11.73
11.74
11.56
11.92
11.51
11.37 11.92
Na
2
O
1.40
1.62
1.86
1.70
1.86
2.24
1.46
1.87
2.26
2.22
2.37
2.24
2.49
2.29
2.20
1.96
K
2
O
0.23
0.32
0.38
0.24
0.48
0.38
1.38
1.38
0.84
0.84
0.75
0.71
0.80
0.69
0.92
0.74
BaO
0.00
0.00
0.01
0.00
0.01
0.00
0.02
0.03
0.03
0.01
0.01
0.00
0.02
0.01
0.01
0.02
F
0.08
0.13
0.14
0.12
0.12
0.00
0.11
0.14
0.21
0.24
0.14
0.08
0.08
0.06
0.21
0.21
Total
97.17
97.27 97.15 96.98 97.08 97.17
97.34
97.19
96.91
96.85
97.84
97.57
98.01
97.47
97.01 97.62
Si
6.51
6.18
6.21
6.35
6.29
6.21
6.21
6.15
6.18
6.20
6.13
6.12
6.14
6.18
6.35
6.34
Al
IV
1.49
1.82
1.79
1.65
1.71
1.79
1.79
1.85
1.82
1.80
1.87
1.88
1.86
1.82
1.65
1.66
T sites
8.00
8.00
8.00
8.00
8.00
8.00
8.00
8.00
8.00
8.00
8.00
8.00
8.00
8.00
8.00
8.00
Al
VI
0.50
0.61
0.55
0.39
0.40
0.37
0.36
0.40
0.44
0.43
0.38
0.37
0.39
0.41
0.49
0.36
Ti
0.10
0.11
0.08
0.12
0.21
0.24
0.17
0.21
0.14
0.13
0.18
0.21
0.16
0.13
0.22
0.24
Cr
0.00
0.01
0.01
0.00
0.01
0.00
0.01
0.01
0.01
0.01
0.01
0.01
0.01
0.00
0.00
0.01
Fe
3+
0.75
0.84
0.94
0.96
0.53
0.65
0.55
0.44
0.48
0.52
0.48
0.50
0.46
0.62
0.20
0.26
Mg
2.65
2.31
2.28
2.50
2.77
2.79
2.09
2.40
3.32
3.42
3.07
2.79
3.34
3.27
2.82
3.02
Fe
2+
1.00
1.12
1.15
1.02
1.09
0.95
1.82
1.54
0.61
0.49
0.88
1.12
0.64
0.57
1.28
1.11
C sites
5.00
5.00
5.00
5.00
5.00
5.00
5.00
5.00
5.00
5.00
5.00
5.00
5.00
5.00
5.00
5.00
Fe
2+
0.20
0.11
0.14
0.17
0.09
0.16
0.01
0.05
0.07
0.06
0.05
0.04
0.05
0.08
0.02
0.04
Mn
0.08
0.06
0.06
0.07
0.03
0.03
0.07
0.04
0.01
0.02
0.03
0.04
0.02
0.02
0.03
0.02
Ca
1.52
1.64
1.57
1.51
1.75
1.60
1.84
1.79
1.82
1.82
1.83
1.83
1.84
1.78
1.80
1.87
Na
0.20
0.19
0.23
0.24
0.13
0.21
0.08
0.12
0.09
0.09
0.09
0.08
0.12
0.14
0.07
B sites
2.00
2.00
2.00
2.00
2.00
2.00
2.00
2.00
2.00
2.00
2.00
0.09
2.00
2.00
2.00
2.00
2.00
Na
0.20
0.27
0.31
0.25
0.40
0.43
0.35
0.44
0.54
0.53
0.58
0.55
0.62
0.53
0.49
0.49
K
0.04
0.06
0.07
0.05
0.09
0.07
0.27
0.27
0.16
0.14
0.14
0.13
0.15
0.13
0.17
0.14
A sites
0.24
0.33
0.38
0.30
0.49
0.50
0.62
0.70
0.70
0.67
0.72
0.68
0.77
0.65
0.66
0.63
OH
1.96
2.63
2.78
1.94
1.94
2.00
2.69
2.60
1.90
1.98
1.94
1.96
1.96
1.97
1.90
1.90
Mg#
0.69
0.65
0.64
0.68
0.70
0.72
0.53
0.60
0.83
0.86
0.77
0.70
0.83
0.87
0.68
0.73
Modif.
ferro
ferro
ferro
ferro
pts
pts
Name
tsch
tsch
tsch
tsch
tsch
tsch
mghas
mghas
mghas
mghas
mghas
mghas
mghas
mghas
parg
parg
PETROGENESIS OF CALC-ALKALINE ROCKS: NEOGENE SUBVOLCANIC AREA (EASTERN CARPATHIANS) 81
rocks and cognate enclaves. Some amphiboles (e.g. Arsente
microdiorite) display Mg-richer core and Fe-richer rim, while
other amphiboles (e.g. Sturzii dacite) display reverse zonation
with Mg-richer rim and Fe-richer core.
Pyroxenes are present only in the more basic petrographic
types, where they are subordinated in abundance to the am-
phiboles. They are also found in some mafic magmatic cog-
nate enclaves. In some cognate enclaves pyroxene is the only
mineralogical component. Only clinopyroxene occurs in the
studied rocks (Table 2). Within the cognate enclaves mostly
diopside is present, while augite occurs mainly in the host-
rocks. Occasionally, clinoenstatite was found in the pyroxen-
ite enclaves within the Arsente microdiorite.
Biotite is present in the more acidic petrographical types ei-
ther as the only mafic mineral (Parva rhyolite) or in associa-
tion with amphiboles (Ilva rhyodacites and dacites, as well as
Valea Vinului quartz biotite andesites). It is also present in the
mafic magmatic cognate enclaves within the Valea Vinului In-
trusive Unit, where it has a slightly different chemical compo-
sition compared with the host-rock biotite. This corresponds
to higher Al and Fe, and to lower Mg content.
Plagioclase feldspars are the main components of all the
petrographic types; they form both phenocrysts and microlites
in the matrix. Anorthite content varies according to the petro-
Sample
Analysis
Location
I5
Rock
Chicera
I4
rock
Arsente
I4/A2
en
Arsente
I4px0
en
Arsente
I4px0
en
Arsente
I4px1
en
Arsente
I4px2
en
Arsente
I4px4
en
Arsente
I14
en
Cornii
I6
en(cor)
Runc
I6
en(rim)
Runc
SiO
2
52.13
52.07
51.12
53.65
55.14
52.54
52.83
52.25
50.67
51.84
51.59
Al
2
O
3
1.56
1.28
3.18
1.77
1.83
1.85
1.52
2.25
3.84
2.08
2.14
TiO
2
0.63
0.28
0.56
0.24
0.13
0.20
0.20
0.11
0.72
0.62
0.58
Cr
2
O
3
0.10
0.07
0.05
0.52
0.34
0.14
0.10
0.00
0.00
0.00
0.00
FeO*
8.17
9.29
6.30
3.92
11.15
5.27
5.46
6.40
6.70
9.44
9.41
MnO
0.48
0.46
0.24
0.20
0.25
0.13
0.24
0.27
0.24
0.37
0.39
MgO
14.69
14.14
15.62
17.03
30.08
15.51
15.21
15.59
13.70
15.22
14.94
CaO
20.86
21.59
21.87
22.50
0.67
24.18
24.00
22.39
23.69
19.97
20.33
K
2
O
0.04
0.03
0.03
0.01
0.01
0.00
0.00
0.00
0.02
0.03
0.02
Na
2
O
0.50
0.25
0.31
0.21
0.02
0.13
0.13
0.30
0.41
0.29
0.27
BaO
0.00
0.03
0.00
0.02
0.00
0.00
0.00
0.00
0.02
0.00
0.00
F
0.11
0.24
0.00
0.03
0.00
0.14
0.20
0.31
0.00
0.00
0.23
Total
99.26
99.72
99.27
100.00
99.60
100.09
99.90
99.90
100.06
99.86
99.91
WO
43.41
44.17
44.90
45.54
1.30
48.39
48.37
45.40
49.19
40.91
41.68
EN
42.53
40.26
44.62
47.95
81.40
43.18
42.66
44.02
39.58
43.39
42.62
FS
14.06
15.57
10.48
6.51
17.30
8.43
8.97
10.58
11.23
15.70
15.70
graphic type: between 2025 % (oligoclase) in acid rocks, and
between 5576 % (labradorbytownite) in most microdiorites
and basaltic andesites (Table 3). The plagioclases in Chicera
and Heniu Magmatic Units (microdiorites, amphibole andes-
ites) are even more basic, with an anorthite content of 70
80 %. Plagioclase feldspars frequently show normal and oscil-
latory zoning, which is best shown in samples of the Arsente,
Valea Vinului, Cornii and Sturzii Units, indicating modifica-
tion of crystallization conditions (i.e. magma chamber refilling
and/or rapid cooling during the emplacement of the intrusive
body).
Potassic feldspars are present in very small amounts (0
4 wt. %), mostly in the cognate enclaves or in the form of mi-
crolites in the matrix of the more acidic petrographic types
(Valea Vinului). They form totally subordinated phenocrysts
in porphyritic microgranodiorites. They are mostly orthoclase.
In many cases they are replaced by sericite, kaolinite and cal-
cite.
Garnets are present only in the Pleºii-Mal quartz andesites
and Sturzii dacite, as 12 wt. % of the rock volume. They
form phenocrysts with subhedral or euhedral morphologies,
0.52.5 mm in size, and have almandine-rich compositions
(over 55 %) (Table 4). Garnets are fresh, without inclusions
and reaction zones. Most are found as inclusions in plagio-
Sample
Analysis
Location
I15
rock
core
Sturzii
I15
rock
middle
Sturzii
I15
rock
rim
Sturzii
I31
rock
Pleºii
I8
rock
Heniu
I8/hb1
en
Heniu
I8/hb2
en
Heniu
I4/A2
en
core
Arsente
I4/A2
en
middle
Arsente
I4/A2
en
rim
Arsente
I4mega
en
Arsente
I6
rock
Runc
SiO
2
55.42
57.43
56.25
57.15
50.97
52.04
64.54
55.40
54.46
56.33
65.03
51.66
Al
2
O
3
27.78
26.38
27.18
26.40
30.56
29.57
18.18
27.23
28.00
26.62
18.31
29.66
CaO
10.29
8.59
9.59
8.71
13.67
12.81
0.17
9.81
10.77
9.31
0.11
13.08
MnO
0.11
0.00
0.00
0.11
0.04
0.03
0.00
0.00
0.00
0.00
0.00
0.04
FeO*
0.14
0.07
0.07
0.09
0.25
0.24
0.16
0.28
0.29
0.29
0.06
0.63
BaO
0.00
0.05
0.04
0.01
0.00
0.03
0.11
0.00
0.06
0.03
0.10
0.00
Na
2
O
5.70
6.65
6.07
6.43
3.75
4.26
0.66
5.93
5.14
6.13
0.39
4.00
K
2
O
0.16
0.15
0.14
0.17
0.07
0.09
15.38
0.38
0.32
0.33
15.99
0.20
Total
99.60
99.33
99.33
99.07
99.34
99.05
99.19
99.03
99.04
99.04
100.00
99.30
Ab
49.59
57.83
52.97
56.60
33.00
37.40
6.00
51.12
45.49
53.32
3.60
35.20
An
49.49
41.29
46.25
42.40
66.50
62.10
0.80
46.71
52.67
44.77
0.00
63.70
Or
0.92
0.88
0.78
1.00
0.50
0.50
93.10
2.17
1.84
1.91
96.40
1.10
Table 3: Representative microprobe analyses of feldspars of host rocks and enclaves. Abbreviation: en enclave.
Table 2: Representative microprobe analyses of pyroxenes of host rocks and enclaves. Abbreviation: en enclave.
82 PAPP, URECHE, SEGHEDI, DOWNES and DALLAI
Table 4: Representative microprobe analyses of garnets. Abbreviations: plz plagioclase; hbl hornblende.
Sample
I9 Mal
Pleºii
Analysis
in plz
in plz (from rim to core)
in hbl
rim
middle
core
1
2
3
4
5
6
rim
middle
core
SiO
2
37.69
37.90
37.90
37.52
37.79
37.70
37.67
37.52
37.55
37.42
37.63
37.71
TiO
2
0.19
0.16
0.06
0.23
0.09
0.13
0.21
0.25
0.28
0.29
0.21
0.18
Al
2
O
3
20.78
20.82
20.87
20.60
20.85
20.58
20.59
20.55
20.81
20.29 20.5
20.75
Cr
2
O
3
0.08
0.00
0.00
0.00
0.00
0.00
0.00
0.08
0.00
0.00
0.00
0.00
MgO
5.81
5.57
5.68
5.60
5.45
5.25
5.05 4.6
5.35
5.35
5.42
5.45
CaO
5.22
5.37
4.51
4.74
5.35
4.66
5.65
4.35
5.11
4.95
4.58
5.13
MnO
3.85
3.45
4.15
4.03
3.59
4.52
3.75
5.22
4.11
3.55
3.99
3.65
FeO
27.35
27.51
27.72
28.14
27.87
28.05
28.03
27.69
27.73
28.36
28.56
28.07
Total
100.97
100.78
100.89
100.86
100.99
100.89
100.95
100.26
100.94
100.20
100.89
100.94
End
members
Uv
0.24
0.00
0.00
0.00
0.00
0.00
0.00
0.24
0.00
0.00
0.00
0.00
Adr
0.53
0.45
0.17
0.63
0.25
0.37
0.59
0.72
0.79
0.80
0.59
0.51
Grs
13.29
13.95
11.91
11.95
14.00
12.08
14.47
11.17
12.86
12.46
11.60
13.17
Alm
56.49
57.53
57.96
58.29
57.97
58.49
58.31
59.09
57.80
59.29
59.34
58.42
Sps
8.06
7.31
8.79
8.46
7.56
9.55
7.90
11.28
8.68
7.53
8.40
7.69
Prp
21.39
20.77
21.17
20.68
20.22
19.51
18.73
17.50
19.87
19.92
20.07
20.21
Sum
100.00
100.00
100.00
100.00
100.00
100.00
100.00
100.00
100.00
100.00
100.00
100.00
clase and rarely in hornblende phenocrysts. Garnets occur ei-
ther in the core of their host crystals or they can have a periph-
eral position. The optical and chemical features of the plagio-
clases hosting garnet crystals are similar to other plagioclases
in the rocks.
The presence of the assemblage amphibole-biotitequartz
plagioclaseK-feldsparmagnetite in lithologies like Sturzii
dacite and Valea Vinului andesites recommend that the Al-
content in hornblende geobarometer of Johnson & Rutherford
(1989) may be applied for pressure estimations. Assuming
temperatures close to the range over which this barometer has
been calibrated (740780 °C) pressures of 550800 MPa have
resulted. The same barometer has been tentatively applied for
others intrusive units (Pleºii, Cornii, Chicera, Arsente, Heniu,
Iliuþa) resulting in pressures within the same range, both for
host-rocks and cognate enclaves. Slightly higher pressure val-
ues have been obtained in the case of cognate enclaves com-
pared with their host-rocks. The highest pressure has been
found for the Sturzii dacite. Significant differences are record-
ed between the pressure values corresponding to the core of
the crystals from Sturzii dacite (~780 MPa) and the pressure
value corresponding to the rim (~490 MPa). This finding im-
plies that decompression occurred during crystallization of
amphiboles. The pressure estimates for host-rocks and cognate
enclaves suggest mid-crustal depths of approximately 15
25 km for amphibole crystallization.
Major and trace element geochemistry
Major and trace elements compositions of the host-rocks
and cognate enclaves are presented in Table 5. SiO
2
ranges be-
tween 39.81 wt. % and 49.87 wt. % in the mafic magmatic
cognate enclaves, and from 52.42 wt. % (Colibiþa andesite) to
75.39 wt. % (Parva rhyolite) in the host-rocks. This variation
corresponds to basalts, basaltic andesites, andesite, dacites and
rhyolite. Two series of rocks can be seen in the K
2
O-SiO
2
dia-
Fig. 2. Si O
2
vs. Na
2
O+K
2
O diagrams for Rodna-Bârgãu igneous
rocks showing the separation of two series of rocks.
gram (LeMaitre 1989) (Fig. 2). The first series comprises
andesites and microdiorites from South Bârgãu (Heniu, Oala),
the quartz garnet andesites (Pleºii-Mal), Sturzii-Bucnitori dac-
ites and Parva rhyolites and lies in the medium- to low-K do-
main. The second series contains some of the basaltic andes-
ites, Mãguri and Cornii andesites and microdiorites, and Valea
Vinului biotite quartz andesites. It trends towards the high-K
field. It is worth noting that within the medium-K series am-
phiboles are the only mafic minerals, while within the high-K
series clinopyroxenes, amphiboles and biotites all occur. The
cognate enclaves fall mostly in the domain of basalts, with
SiO
2
less than 50 wt. %, and K
2
O less than 1 wt. %, except
those from the Valea Vinului and Arsente which are enriched
in K
2
O due to high biotite content.
PETROGENESIS OF CALC-ALKALINE ROCKS: NEOGENE SUBVOLCANIC AREA (EASTERN CARPATHIANS) 83
Isotopic composition of the magmatic rocks
Table 6 summarizes the oxygen and strontium isotope anal-
yses performed on host-rocks and cognate enclaves from the
main intrusive units. Mineral separates, mostly amphibole and
pyroxene, were analysed for O isotope ration because whole-
rock δ
18
O values can often be affected by low-temperature
processes such as hydration and weathering, which are charac-
terized by large
18
O enrichment effects.
Our samples display δ
18
O values between 3.7 and 6.7
(SMOW). These values are lower than the expected values for
pyroxene and hornblende in typical continental margin arc
volcanic rocks (e.g. Hoefs 1997). The variation of δ
18
O values
reported for the neighbouring areas (Neogene magmatites
from CãlimaniGurghiu-Harghita Mountains (Mason et al.
1996)) and Ukrainian Neogene volcanic arc (Seghedi et al.
2001) is clearly different (5.1 to 8.7 and 6.1 to 8.3 re-
spectively) (see also Fig. 7).
Using mineralogical (clinopyroxene vs. amphibole), petro-
graphical (xenolith vs. host-rock) and geochemical (medium-
Fig. 3a. Major and trace element for Rodna-Bârgãu igneous rocks.
Symbols as in Fig. 2.
Fig. 3b. Harker variation diagrams for Rodna-Bârgãu igneous rocks.
Symbols as in Fig. 2.
In the host rocks, variation trends of TiO
2
, FeO*, MgO, and
CaO with SiO
2
content show negative correlations, whereas
K
2
O and Na
2
O increase with increasing SiO
2
(Fig. 3a). The
major element variation of the cognate enclaves is more scat-
tered. The compatible trace element contents (Ni, Cr, Co) are
higher in the cognate enclaves compared with the host rocks
(Table 5). The variation with SiO
2
of these elements is con-
trasting in cognate enclaves (increasing as SiO
2
increases) and
in host-rocks (decreasing as SiO
2
increases). A better correla-
tion was obtained for host-rocks as compared to cognate en-
claves. Rb, Nb, Pb, Sr, Zr and Y show a scattered variation
with SiO
2
(Fig. 3b). The two series of rocks distinguished ac-
cording to the K
2
O-SiO
2
diagram are also discriminated on the
Rb-SiO
2
variation diagram. The variation of Y in cognate en-
claves clearly exceeds that of the host-rocks. The Sr and Zr
contents in cognate enclaves are slightly lower than in the
host-rocks.
The incompatible trace elements and the REE compositions
are similar for both host-rocks and cognate enclaves (Table 5).
However, the cognate enclaves are less enriched in incompati-
ble trace elements and more heterogeneous than the host-
rocks. The REE patterns of rocks (Fig. 4) correspond to those
from arcs associated with subduction areas (Wilson 1989) and
resemble the neighbouring areas of the Carpathian arc
(Downes et al. 1995; Mason et al. 1996). They are LREE en-
riched, while the HREE pattern is similar to the primitive
mantle.
Fig. 4. Chondrite-normalized rare earth elements diagram for repre-
sentative rocks. Normalized coefficient from Sun & McDonough
(1989). Symbols as in Fig. 2 and sample names as in Table 5.
84 PAPP, URECHE, SEGHEDI, DOWNES and DALLAI
Table 5: Major and trace element data for Rodna-Bârgãu igneous rocks. Major elements are given in percent (%) and trace elements in ppm.
Abbreviations: ba basaltic andesite; pa pyroxene andesite; aa amphibole andesite; qba quartz biotite andesite; qga quartz
garnet andesite; md microdiorites; d dacite; r rhyolite; nd not determined. Total iron is expressed as FeO.
Sample
Location
Rock type
P1
Parva
r
P2
Parva
r
P3
Parva
r
I15
Sturzii
d
P21
Sturzii
d
P22
Bucnitori
d
P23
Bucnitori
d
I10
V.Vin.
qba
I11
V.Vin.
qba
P13
V.Vin.
qba
P14
V.Vin.
a
P4
Plesii
qga
I9
Mal
qga
I14
Cornii
aa
P82
Cornii
aa
P108
Cornii
aa
I4
Arsente
md
P62
Arsente
md
I5
Chicera
md
P71
Chicera
md
SiO
2
75.39 74.17 74.52 65.30 67.22 66.53 67.27 60.33 61.42 63.95 63.22 64.92 58.60 58.23 59.36 58.17 54.50 55.93 53.12 54.23
TiO
2
0.17 0.05 0.12 0.34 0.33 0.20 0.52 0.49 0.58 0.54 0.64 0.45 0.66 0.64 0.51 0.61 1.04 0.92 0.47 0.84
Al
2
O
3
14.53 15.18 15.26 17.30 16.16 16.14 16.98 15.01 16.69 16.07 16.14 16.98 18.97 18.4 17.74 16.53 17.77 18.14 19.96 17.69
FeO*
1.41 1.25 1.65 3.87 3.40 3.13 3.33 6.83 5.70 6.45 5.49 4.15 5.07 8.43 6.31 7.23 8.24 6.23 5.43 7.54
MnO
0.07 0.06 0.04 0.11 0.10 0.09 0.09 0.24 0.13 0.11 0.13 0.09 0.16 0.15 0.14 0.17 0.24 0.14 0.05 0.14
MgO
0.20 0.30 0.20 1.44 1.38 1.26 0.86 3.68 2.73 2.43 2.45 2.27 1.98 2.62 2.7 3.52 4.28 4.14 4.62 4.78
CaO
1.49 1.41 1.98 5.17 5.06 5.58 3.87 5.88 4.68 0.07 5.41 4.71 6.83 6.01 6.47 6.41 7.18 7.25 9.45 8.84
Na
2
O
2.10 2.25 3.23 3.59 3.89 4.11 4.05 2.8 3.13 3.83 3.31 4.05 3.4 3.14 4.15 3.64 3.32 3.58 3.05 3.05
K
2
O
3.50 3.47 2.32 0.96 1.39 1.86 1.81 2.88 3.24 3.24 2.95 1.15 0.93 1.81 2.35 2.66 2.07 1.89 2.75 1.56
P
2
O
5
0.05 0.04 0.16 0.26 0.09 0.08 0.10 0.23 0.3 0.60 0.27 0.09 0.02 0.16 0.20 0.21 0.23 0.18 0.06 0.18
H
2
O
2.36 2.17 1.28 0.95 1.14 1.41 1.30 0.89 1.11 1.97 0.66 1.68 2.9 0.18 0.90 1.00 1.63 1.77 1.12 1.41
Total
100.27 100.35 100.76 99.29 100.16 100.39 100.18 99.26 99.71 99.26 100.67 100.54 99.52 99.77 100.83 100.15 100.50 100.17 100.08 100.28
Rb
189
nd 128
39 61 71
67
120
111
118 115
51
35
66 81 71
63
51
54
62
Sr
173 207 225
287 386 325
351
420
393
288 345
368
287
435
482 358
386
235
333
207
Y
14 11
nd 15
nd 10
19
25
24
22 23
20
16
24 30 20
16
nd 17
21
Zr
39 44 67
111 137 101
103
168
156
150 188
123
110
145
162 138
109
nd 96
73
Nb
nd
nd
nd 11
nd
nd
nd 10
10
nd
nd
nd
9
5
nd
nd 4
nd 5
nd
Pb
21 42 13
3 4
nd
6
12
18
24 14
3
5
11 15 13
36
20
58
16
Ga
8
nd 11
15 15
nd 12
29
17
19 21
18
18
16 16 16
21
25
6
15
Zn
nd 52 47
45 42
nd 45
78
120
125 73
92
90
71 114
41
nd 59
Ni
4 5 7
6 7
nd
5
13
15
15 10
19
12
16 10 12
27
22
4
51
Co
1 5 3
4 5 5
5
11
9
11 9
7
10
17
7 14
18
11
11
33
Ba
325 601 378
220 376 403
516
1023
1010
746 993
307
300
844
772 821
426
327
95
246
Cr
5 6 10
11 10 10
19
43
40
84 84
11
46
36 32 21
38
92
253
236
V
14 23 18
45 66
nd 36
122
112
108 136
72
75
153
122 132
179
107
150
226
Sc
nd
nd
nd 8 10 6
6
13
15
12 15
10
12
23 12 28
17
nd
9
nd
Cu
65 13 20
22 10
nd
8
36
20
39 31
38
23
34 38 35
76
53
46
65
Sn
nd
nd
nd
nd 2.03
nd 2.06 1.14 2.00 2.06 2.09 nd 2.50 2.00 2.02 nd
nd
nd
nd
nd
La
23.77 24.89 nd 25.00 30.49 17.25 33.03 36.00 31.00 43.27 62.70 17.91 12.00 39.00 53.65 32.56 14.60 nd 3.80
nd
Ce
26.70 nd
nd 31.00 nd 31.45
nd
nd
nd
nd
nd 23.03 18.00 29.00 29.36 nd 13.30 nd 4.80
nd
Sm
3.35 nd
nd 4.33 nd 4.36
nd
nd
nd
nd
nd 2.76 4.40 4.20 4.25 nd 3.8
nd 1.30
nd
Eu
0.85 nd
nd 0.43 nd 0.44
nd
nd
nd
nd
nd 0.82 0.75 0.37 0.37 nd 0.84 nd 0.51
nd
Tb
0.45 0.93 nd 0.46 nd 0.16
nd
nd
nd
nd
nd 0.55 0.52 0.69 0.37 nd 0.38 nd 0.43
nd
Yb
0.61 nd
nd 1.20 1.63 0.88 1.45 2.40
nd 2.47 2.61 1.35 1.58 2.38 1.55 2.54 0.67
nd 0.79
nd
Lu
nd
nd
nd 0.27 nd 0.27
nd
nd
nd
nd
nd 0.17 0.24 0.12 0.12 nd
nd
nd
nd
nd
Cs
9.42 nd
nd
nd
nd 0.51
nd
nd
nd
nd
nd 0.31 nd 2.80 nd
nd 1.20 nd
nd
nd
Th
10.16 nd
nd 4.40 nd 4.46
nd 11.00 11.10 11.64 11.49 1.64 1.00 4.00 4.05 nd 4.30 nd
1.60
nd
Hf
1.99 nd
nd 2.60 nd
nd
nd
nd
nd
nd
nd 1.54 1.50 2.50 nd
nd
nd
nd
nd
nd
Ta
2.41 nd
nd 1.20 nd
nd
nd
nd
nd
nd
nd 1.02 0.50 1.40 nd
nd
nd
nd
nd
nd
K vs. high-K series) criteria, several groups of δ
18
O values
have been delimited. Descriptive statistics of the δ
18
O values
is presented in Table 7. For comparison, the variation of the
δ
18
O values in mantle clinopyroxenes (amphiboles present) is
also shown (data from Mattey et al. 1994). To test for signifi-
cant differences between means, one-way analysis of variance
test (ANOVA) has been performed giving p=0.0026 (differ-
ences are significant at p<0.05). The pyroxenes from cognate
enclaves show the closest values to the mantle. Comparable
values were found in Iliuþa basaltic andesite. The lowest val-
ues are shown by the Mãguri andesites (high-K series). The
highest δ
18
O values were found in the Cornii (6.6 ) and
Colibiþa andesites (6.7 ). The most scattered values are
shown by amphiboles from the cognate enclaves. In some of
the analysed enclaves (I4px1, I4px2, I4px4, I8/hb2) isotopic
disequilibria between amphiboles and coexisting pyroxenes
can be observed.
The δ
18
O value for garnet from the Pleºii quartz garnet
andesite (4.3 ) lies within the range of the δ-values exhibit-
ed by the amphiboles from the medium-K series. Much higher
δ
18
O value (7.3 ) was obtained for the metamorphic garnet
(alm 61 %; and 23 %; sps 4 %; prp 12 %) from the staurolite
garnet micaschists within the Rebra series. The δ
18
O value of
the Pleºii garnet is lower than the values for garnet reported in
the literature (Harangi et al. 2001 and literature there in). For
the Carpatho-Pannonian region the δ
18
O values of the igneous
almandine garnet range from 6.1 to 10.5 (Mason et al.
1996; Harangi et al. 2001).
Age correction of the measured
87
Sr/
86
Sr ratio values (using
data from Pécskay et al. 1995) has been performed in order to
PETROGENESIS OF CALC-ALKALINE ROCKS: NEOGENE SUBVOLCANIC AREA (EASTERN CARPATHIANS) 85
Table 5: Continuing.
Sample
Location
Rock type
P95
Chicera
md
I6
Runc
pa
P11
Heniu
aa
I8
Heniu
aa
I7
Oala
aa
I16
Colibita
aa
I18
Iliuþa
ba
Cognate
enclave
I10/en
V.Vin.
I14/en
Cornii
I4/A2
Arsente
I4/A3
Arsente
I4 px0
Arsente
I4 px 1
Arsente
I4 px 4
Arsente
I5/en
Chicera
I8/hb2
Heniu
I8/hb1
Heniu
I16/en
Colibita
SiO
2
56.93 52.46 52.83 53.08 58.96 52.42 53.78 SiO
2
47.91 41.68 48.62 42.52 49.87 46.97 47.05 39.81 43.31 42.33 47.62
TiO
2
0.65 0.93 1.07 1.12 0.67 0.72 0.95 TiO
2
1.73 1.86 1.29 1.17 0.35 0.73 0.69 2.00 1.67 1.40 1.23
Al
2
O
3
17.51 17.02 18.78 18.15 17.82 18.94 18.76 Al
2
O
3
16.65 13.98 14.05 13.25 2.42 7.00 6.35 16.66 12.25 13.70 17.75
FeO*
6.27 7.98 10.60 8.17 5.86 9.21 7.69 FeO* 13.47 14.15 11.13 10.43 6.63 9.06 8.85 16.20 11.34 11.95 10.66
MnO
0.10 0.17 0.17 0.26 0.15 0.18 0.17 MnO 0.29 0.31 0.21 0.18 0.12 0.16 0.15 0.21 0.19 0.14 0.17
MgO
4.15 6.31 3.27 3.49 2.69 3.56 4.93 MgO 6.55 11.50 10.23 14.89 19.56 16.42 16.98 9.09 13.86 14.17 7.34
CaO
8.15 10.81 8.57 7.69 6.17 6.88 6.90 CaO 5.19 10.16 9.23 11.53 19.83 17.31 17.81 11.34 12.98 11.52 9.51
Na
2
O
3.42 2.76 3.56 3.81 3.88 3.91 3.89 Na
2
O 2.45 1.99 1.88 2.33 0.31 0.93 0.82 1.98 1.60 2.08 2.77
K
2
O
1.69 1.37 1.00 1.34 1.18 1.12 1.06 K
2
O
3.3 1.17 2.31 0.68 0.04 0.33 0.28 0.39 0.87 0.76 0.81
P
2
O
5
0.14 0.12 0.13 0.14 0.19 0.2 0.17 P
2
O
5
0.12 0.19 0.06 0.1 0
0.09 0.02 0.11 0.05
0
0.06
H
2
O
1.67 0.96 0.75 2.10 2.11 2.06 1.07 H
2
O 2.56 2.25 1.00 2.26 0.89 1.00 1.00 1.88 1.77 2.11 1.94
Total
100.68 100.89 100.73 99.35 99.68 99.20 99.37 Total 100.22 99.24 99.34 73.39 100.02 100.00 100.00 99.67 99.89 100.16 99.89
Rb
57
46
50 29 16 69
42
Rb
157 11
81
19
2
2
4
19
37
7
80
Sr
319
454
472
256 210 442
327
Sr
220 129
195
154
41
83
77
163
94
127
190
Y
14
16
40 23 17 22
22
Y
39 28
23
18
5
14
14
18
30
21
47
Zr
102
94
181
116 73 143
146
Zr
58 48
85
44
13
25
20
40
56
40
120
Nb
nd 6
10 9 4 6
8
Nb
16 4
4
3
3
3
3
3
8
4
10
Pb
8
27
4 14 2 3
5
Pb
17 16
7
11
9
6
5
14
6
4
3
Ga
21
27
19 16 18 17
19
Ga
32 26
14
14
20
11
10
13
13
13
22
Zn
74
nd 77
nd
nd 57
nd
Zn
nd
nd 73
217
nd 42
37
nd
nd
nd
nd
Ni
20
17
14 24 2.5 8
35
Ni
17 19
72
82
15
109
109
65
77
80
23
Co
18
33
22 22 9 10
32
Co
65 21
53
54
23
72
54
32
30
35
58
Ba
432
460
231
310 550 270
240
Ba
1000 0
584
210
19
77
70
40
nd 0
115
Cr
70
35
48 320 44 19
130
Cr
6 70
111
38
60
378
370
nd 80
58
38
V
237
340
191
320 120 160
240
V
300 28
411
334
300
273
267
320
450
330
440
Sc
26
34
28 25 11.7 15
28
Sc
90 15
nd
nd 22
nd
nd 0
90
280
80
Cu
62
210
32 35 32 43
110
Cu
210 50
nd
nd 43
nd
nd 63
65
62
310
Sn
nd
nd 21 2 2.5
nd 3
Sn
5.5 3
nd
nd 0
nd
nd 0
3
3
2
La
nd
nd 11.41 11.43 31.31 13.85 30.00 La
<30
nd <30
<30
<30
<30
<30
30
nd
nd
nd
Ce
nd
nd 10.40 10.42 29.71 11.68
nd
Ce
nd
nd 37
39
nd 37
30
nd
nd
nd
nd
Sm
nd
nd 2.61 2.65 5.82 3.00
nd
Sm
nd
nd
nd
nd
nd
nd
nd
nd
nd
nd
nd
Eu
nd
nd 0.73 0.73 1.32 0.78
nd
Eu
nd
nd
nd
nd
nd
nd
nd
nd
nd
nd
nd
Tb
nd
nd 0.55 0.55 0.57 0.45
nd
Tb
nd
nd
nd
nd
nd
nd
nd
nd
nd
nd
nd
Yb
nd 3.00 2.61 1.85 0.64 1.55 3.00 Yb
7 3
nd
nd
nd
nd
nd
nd
nd
nd 5
Lu
nd
nd
nd
nd 0.13 0.16
nd
Lu
nd
nd
nd
nd
nd
nd
nd
nd
nd
nd
nd
Cs
nd
nd 1.91 nd 2
nd
nd
Cs
nd
nd
nd
nd
nd
nd
nd
nd
nd
nd
nd
Th
nd 4.30 2.71 2.73 12.21 4.00 10.00 Th
nd
nd 3
<2
nd <2
<2
nd
nd
nd
nd
Hf
nd
nd 2.01 nd
nd
nd
nd
Hf
nd
nd
nd
nd
nd
nd
nd
nd
nd
nd
nd
Ta
nd
nd 0.53 nd
nd
nd
nd
Ta
nd
nd
nd
nd
nd
nd
nd
nd
nd
nd
nd
obtain the initial
87
Sr/
86
Sr ratios (Table 6). The differences be-
tween corrected and uncorrected values are negligible. The
initial
87
Sr/
86
Sr ratios have been used in all diagrams. The total
range of
87
Sr/
86
Sr ratios is from 0.70588 to 0.70950. The low-
est value is from the Iliuþa basaltic andesite from the medium-
K series. Variation curves of the host-rocks from medium-K
and high-K series plot as distinctive straight lines on the
87
Sr/
86
Sr vs. 1/Sr diagram (Fig. 5), suggesting two-component
mixing. The increase of the
87
Sr/
86
Sr ratios matches the in-
crease of the Sr content in the high-K series. For the medium-
K series there is a slightly negative correlation between the
two parameters. The cognate enclaves display
87
Sr/
86
Sr ratios
from 0.70620 to 0.70902. On the
87
Sr/
86
Sr vs. 1/Sr diagram,
the pyroxenites and the hornblendites define distinct fields.
There is a larger variation of Sr content within the cognate en-
claves than in the host rock. The similar
87
Sr/
86
Sr signature of
the cognate enclaves as compared with their host rocks is con-
sistent with their co-magmatic origin. In some cases higher
values were found in cognate enclaves relative to their host
rock. This could be explained by their relatively low Sr con-
Fig . 5.
87
Sr/
86
Sr vs. 1/Sr for host-rocks and cognate enclaves in the
Rodna-Bârgãu Mountains.
tent (41 to 195 ppm) that made them more susceptible to
87
Sr
contamination.
86 PAPP, URECHE, SEGHEDI, DOWNES and DALLAI
Discussion
The results of the geochemical study based on the major,
minor, rare earth elements, O and Sr isotopes can be used to
form a framework for discussion of the petrogenetic processes
that influenced the magma evolution in the region.
Processes related to magma differentiation
Differentiation by fractional crystallization is suggested by
the existence of a complete series of rocks containing all the
petrographic types, from basalts to rhyolites. The presence of
a great variety of mineral species: plagioclases, amphiboles,
pyroxenes, quartz, biotite, garnets, iron oxides etc. corre-
sponds to a succession of fractional crystallization. The pres-
ence of obvious trends of linear correlation of the major ele-
ments with differentiation indices (SiO
2
) also pleads for
magma differentiation (Fig. 3a). Another argument for frac-
tional crystallization is offered by the REE pattern. The nega-
tive anomaly of Eu found in all lithologies indicates the im-
portance of plagioclase fractionation. The negative Eu
anomaly could also be generated by partial melting with a pla-
gioclase-rich residue. Scattered variations of minor elements
with SiO
2
, indicate diverse conditions of differentiation for
Series
Sample
Location
Rock type
87
Sr/
86
Sr
87
Sr/
86
Sr
i
ä
18
O
cpx
ä
18
O
hbl
ä
18
O
grt
medium-K
I15
Sturzii
dacite
0.70818
0.70812
4.3
I9
Mal
qtz grt andesite
0.70704
0.70699
I31
Pleºii
qtz grt andesite
4.8
4.3
I7
Oala
amph andesite
0.70671
0.70668
5.2
I8
Heniu
amph andesite
0.70929
0.70925
4.8
I8/hb1
Heniu
hornblendite
0.70798
0.70796
5.1
I8/hb2
Heniu
hornblendite
0.70902
0.70887
4.2
I18
Iliuþa
basaltic andesite
0.70593
0.70588
5.4
high-K
I10
V.Vinului
qtz bi andesite
0.7090
0.70889
I11
V.Vinului
qtz bi andesite
0.70749
0.70738
I4
Arsente
microdiorite
0.70797
0.70791
3.9
I4/A2
Arsente
hornblendite
0.70620
0.70605
3.8
I4mega
Arsente
hornblendite
0.70954
0.70950
4.6
I4px0
Arsente
pyroxenite
0.70862
0.70860
5.7
I4px1
Arsente
pyroxenite
0.70633
0.70632
5.2
4.2
I4px2
Arsente
pyroxenite
0.70879
0.70877
4.6
5.2
I4px4
Arsente
pyroxenite
0.70941
0.70939
4.6
4.0
I5
Chicera
microdiorite
0.70706
0.70700
4.6
3.7
I5en
Chicera
hornblendite
5.4
I14
Cornii
amph andesite
0.7090
0.70891
6.6
I14en
Cornii
hornblendite
5.7
5.6
I6
Runc
px andesite
0.70794
0.70790
5.3
I16
Colibiþa
amph andesite
0.70845
0.70839
6.7
I16en
Colibiþa
hornblendite
5.2
Rebra
5/96
Rodna
micaschist
7.3
Table 6: Sr-O isotope analyses for representative host-rocks and cognate enclaves from the Rodna-Bârgãu Mountains. Sr isotope data are
expressed as measured and age (10.68.6 Ma) corrected
87
Sr/
86
Sr ratios.
different magmatic units. Consequently, each intrusive unit
may have encountered specific differentiation processes and
possibly did not evolve from a single source.
Similarities in mineralogy of the main mineral species, in P-T
conditions of amphibole crystallization, in incompatible trace
element patterns, and in strontium and oxygen isotope compo-
sition between cognate enclaves and their host rocks, clearly
indicate that cognate enclaves formed from the same magmat-
ic source. They could be products of magma mixing processes
resulting from repeated feeding of magma chambers with pa-
rental mafic melts. This could also explain why cognate en-
claves predominantly occur within larger intrusive units with
intermediate composition (Heniu, Mãguri, Cornii, and Valea
Vinului). The maintenance of an intermediate composition
during crystallization and crustal rock assimilation involves
new inputs of mafic magma. Oscillatory zoning and corrosion
shown by plagioclase phenocrysts from Arsente, Valea Vinu-
lui and Cornii intrusions might also indicate refill of the mag-
matic chamber with less evolved melts. However, an alterna-
tive possible explanation is that the cognate enclaves represent
broken fragments of cumulate layers formed on the floor of
the intermediate magma chambers.
Evidence for crustal assimilation
In subduction-related magmatism possible contamination
mechanisms are: source contamination related to the descend-
ing slab and its sediments, and/or crustal contamination within
crustal magma chamber achieved by assimilation-fractional
crystallization processes (AFC). The existing geotectonic
models in the Carpatho-Pannonian region (e.g. Rãdulescu &
Sãndulescu 1976; Csontos 1995) consider that during the sub-
duction process oceanic crust, thinned continental crust, as
well as related sediments (present-time External Carpathian
Flysch strata) were consumed.
Mantle
Cognate
enclaves
Medium-K
series
High-K
series
Cornii/Colibiþa
cpx
cpx
amph
amph
cpx amph
amph
Mean
5.52
5.30 4.53
4.92
4.95 3.80
6.65
Min.
5.25
4.6
3.8
4.3
4.6 3.7
6.6
Max.
5.75
5.7
5.6
5.4
5.3 3.9
6.7
Std. dev. 0.16
0.52 0.76
0.42
0.49 0.14
Table 7: Summary of the distribution of the δ
18
O values.
PETROGENESIS OF CALC-ALKALINE ROCKS: NEOGENE SUBVOLCANIC AREA (EASTERN CARPATHIANS) 87
High
87
Sr/
86
Sr ratios are usually interpreted in terms of
crustal assimilation. As the increase of the
87
Sr/
86
Sr ratios is
also linked to the enrichment of lithophile trace elements as
compared to primitive mantle and MORB, crustal assimilation
process is to be considered in the petrogenesis of the Rodna-
Bârgãu magmatites. Crustal assimilation is also proved by the
presence of crustal enclaves (metamorphic and sedimentary
rocks).
The Th/Nb vs. SiO
2
diagram (Fig. 6) clearly shows discrim-
ination of the two series of rocks. The high-K series is charac-
terized by higher Th/Nb ratio suggesting a more important
contribution of the upper crust and/or sediments in their gener-
ation, whereas the medium-K series display lower Th/Nb ra-
tios is, therefore, less affected by contamination with such
components.
For the medium-K series the most probably contaminant is
the lower crust. Its involvement is supported by the presence
of garnet-bearing andesites. Petrogenesis of primary garnet-
bearing igneous rocks requires special composition and P-T
conditions of the magma, as well as special tectonic setting for
facilitating rapid ascent of the magma to the surface because
of the limited stability field of the garnet. It is explained by
partial melting of the lower crust due to the uprising of man-
tle-derived magmas, producing small volumes of acid rocks
with a high content of Al
2
O
3
(e.g. Harangi et al. 2001). The
assemblage garnet+plagioclase+amphibole+quartz is stable
at pressures higher than 800 MPa and temperatures of 800
850 °C in a dacite melt with 5 % H
2
O (Day et al. 1992). Such
highly hydrated dacite magma can be generated from a basal-
tic precursor with 23 % water (Green 1992). For the garnet
bearing andesites (Pleºii-Mal) and dacites (Sturzii) high inter-
nal pressure of the magma due to a high H
2
O-rich fluid con-
tent, and the appearance of a decompression regime could fa-
cilitate relatively rapid ascent of magma and preservation of
garnets. The occurrence of the Rodna-Bârgãu garnet-bearing
rocks close to the Someº Fault and the lack of cognate en-
claves, which would indicate the existence of intermediate
chambers, are other arguments for a rapid ascent of magma. A
hydrous mantle source, which is another essential requirement
for the formation of primary garnet-bearing rocks, is consis-
tent with the elevated Ba/La ratio of the rocks from the medi-
um-K series and also with the exclusive occurrence of hydrous
mafic minerals within this series. Exploded fluid inclusions,
surrounded by other small fluid inclusions, found within
quartz grains from Bucnitori dacite, clearly suggest that de-
compression took place (Papp et al. 2003) facilitating rapid as-
cent of magma and preservation of garnets. Pressure decreas-
ing, inferred from the chemical composition of amphiboles in
Sturzii dacite, also suggests a decompression regime.
Significance of the low oxygen isotope ratios
Different processes could induce depletion in
18
O of the
magmatic rocks. Typically, low-
18
O rocks are interpreted in
terms of hydrothermal alteration in the upper crust by interac-
tion with cold meteoric water or seawater. Low temperature
(between 200 and 400 °C) hydrothermal systems with short
lifetimes (<10
6
years) produce large isotopic effects and im-
portant isotopic disequilibrium between rock-forming miner-
als. Other mineralogical and petrographic effects typically oc-
cur (Taylor 1974): partial or total alteration of primary mafic
minerals, micrographic intergrowths of alkali feldspar and
quartz, miarolitic cavities and veins filled with quartz, alkali
feldspar, chlorite, etc. Conversely, sub-solidus hydrothermal
exchange at very high temperatures (400800 °C) is compati-
ble with the general absence of hydrous alteration products in
the mineral assemblages, with the presence of clinopyroxenes,
and with a relatively uniform oxygen isotope composition in
all lithologies (Hoefs 1997 and literature therein). In certain
cases, low-δ
18
O magmas may be formed by remelting of hy-
drothermally altered country rocks or by large-scale assimila-
tion of such material.
Hydrothermal alteration products are poorly developed or
absent in most of the intrusive bodies under study. δD values
measured on whole-rocks (andesites, microdiorites, rhyolites)
or amphiboles vary from 55 to 75 (Papp 1999) and
are normal values for igneous rocks. Because of the high
diffusion rate of hydrogen in rocks, late low-temperature inter-
action with crustal fluids would have produced important
shifts towards low δD values. All these observations, as well
as the existence of a correlation between oxygen and stron-
tium isotopic ratios, lead us to discuss the low measured δ
18
O
values in terms of primary isotopic characteristics of the pa-
rental magmas. However, sub-solidus exchange with meteoric
underground water has to be taken into consideration as a
complementary process during the cooling history of the
rocks, also leading to depletion in
18
O.
On the
87
Sr/
86
Sr vs. δ
18
O diagram (Fig. 7), the medium-K
series defines a significant negative correlation (correlation
coefficient, r=0.72). The trend starts from basaltic andesites
(Iliuþa) to andesites (Oala), quartz andesites (Pleºii-Mal) and
dacites (Sturzii). The decrease of the δ
18
O values as
87
Sr/
86
Sr ra-
tios and SiO
2
increase is interpreted as a progressive contamina-
tion of a mantle-derived magma with a contaminant depleted in
Fig. 6. Th/Nb vs. SiO
2
diagram for Rodna-Bârgãu magmatites.
Flysch sediments (SED) and upper crust (UC) from Mason et al.
(1996), lower crust (LC) from Kempton et al. (1997). Different
fields for cognate enclaves, medium-K and high-K series are
shown. Symbols as in Fig. 2.
88 PAPP, URECHE, SEGHEDI, DOWNES and DALLAI
δ
18
O and enriched in
87
Sr/
86
Sr (i.e. hydrothermally altered crust-
al rocks). As shown in the previous paragraph lower crust could
be taken into consideration as the crustal component. A lower
crust characterized by low δ
18
O values (<4.3 ) and medium
to high
87
Sr/
86
Sr ratios (>0.710) has to be assumed in order to
explain the isotopic characteristic of these rocks. Kempton et al.
(1997) reported similar low δ
18
O values for the lower crust in
the Carpatho-Pannonian area, although they correlate with
much lower
87
Sr/
86
Sr ratios (see Fig. 7).
Iliuþa basaltic andesite is the least contaminated rock, show-
ing δ
18
O values and
87
Sr/
86
Sr ratios close to a mantle source.
Taking into account its volcanic-like texture and the small vol-
ume of the intrusion, we can assume that the magma solidified
rapidly near the surface, without important interaction with
meteoric water to affect the initial δ
18
O value.
The petrogenesis of primary garnet-bearing rocks (Pleºii-
Mal and Sturzii) imply a rapid ascent of magmas, without sig-
nificant contamination within the middle/upper crust. Garnet
is a highly refractory mineral to oxygen isotope exchange. In
the Pleºii andesite the garnet appears to be in isotopic equilib-
rium with the coexisting amphibole (4.8 ). Equilibrium oxy-
gen fractionation between garnet and amphibole is less than
0.4 in the temperature range of 8501000 °C (Zheng 1993a,b).
Moreover, the garnets of the Pleºii andesite display a signifi-
cantly different δ
18
O value compared with the garnets of the
Rebra series (7.3 ) and therefore a xenocrystic metamorphic
origin for the garnets from the quartz andesite could be ruled
out suggesting a primary magmatic origin. Taking all these
facts into consideration, the garnets of the Pleºii andesite
could be indicative for the oxygen isotope composition of the
magma from which it crystallized (i.e. 4.3 ).
In spite of its more basic composition relative to the Pleºii
quartz andesite and Sturzii dacite, Heniu amphibole andesite
exhibits higher
87
Sr/
86
Sr ratios and higher δ
18
O value. A pro-
cess of assimilation and equilibrium crystallization (AEC)
(Huppert & Sparks 1985) could be a possible explanation for
the increasing
87
Sr/
86
Sr. Hotter and voluminous mafic mag-
mas are able to assimilate more crustal material than cooler
less voluminous acid ones. The preservation of an intermedi-
ate composition during assimilation and crystallization im-
plies new inputs of mafic magma, which are supported by the
presence of cognate enclaves (Heniu is by far the largest intru-
sive unit).
Within the high-K series a correlation between the δ
18
O val-
ues,
87
Sr/
86
Sr ratios and SiO
2
content cannot be identified
(Fig. 7). For the Mãguri andesites the distribution is scattered.
In addition, oxygen isotope disequilibrium between coexisting
pyroxenes and amphiboles, both in host-rocks and cognate en-
claves have been observed, as well as additional mineralogical
and petrographical alteration effects (some alteration of prima-
ry mafic minerals, miarolitic cavities and veins filled with
quartz and calcite). These features are characteristics of hydro-
thermal systems with a short lifetime. Therefore, for the
Mãguri intrusions the most probable explanation for the deple-
tion in
18
O is the interaction between intrusive bodies and
heated meteoric water. However, the isotopic heterogeneities
observed within the Mãguri andesites might be due to an inho-
mogeneous source. This could be an incompletely homoge-
nized MASH zone (mixing, assimilation, storage and homoge-
nization; Hildreth & Moorbath 1988), which operated at the
lower-crustal depths. The presence of MASH zones was previ-
ously suggested for the CãlimaniGurghiuHarghita segment
(Mason et al.1996).
Cornii and Colibiþa andesites, from the high-K series, are
characterized by the highest δ
18
O (6.7 ) and
87
Sr/
86
Sr ratio
(0.709), which imply extensive crustal assimilation. These
rocks are well crystallized, and have high K and Sr contents.
They form large intrusions. All these features can be explained
by stagnation of magma in large chambers, situated in the
mid-crustal depth, where AFC processes took place. Distinc-
tive equilibrium mantle-like δ
18
O values of the pyroxene and
amphibole from the cognate enclaves within Cornii andesite
indicate an origin from a mantle-derived uncontaminated
source. The higher δ
18
O values of the host rocks are not con-
sistent with assimilation of a highly altered crust.
Conclusions
The geotectonic evolution and the magmatic processes in
the Rodna-Bârgãu Mountains are an intrinsic part of the gen-
eral evolution of the Carpatho-Pannonian region during Ter-
tiary times. The East Carpathian magmatic arc is closely relat-
ed to the subduction processes located at the southwestern
border of the Eurasian plate.
The results of the mineralogical and geochemical study (ma-
jor and trace elements, oxygen and strontium isotopes) allowed
us to evaluate the petrogenetic processes which influenced mag-
matic evolution. Each intrusive unit encountered specific differ-
entiation processes by fractional crystallization, crustal assimi-
lation and magma mixing. Two different series of rocks have
been separated: one medium-K and another high-K.
Fig. 7. δ
18
O (mineral separate) vs.
87
Sr/
86
Sr (whole-rock) diagram
for Rodna-Bârgãu igneous rocks. Bulk rock fields of Pannonian Ba-
sin lower crust (LC) (Kempton et al. 1997) and for East Carpathian
arc including CãlimaniGurghiuHarghita segment (CGH) (Mason
et al. 1996) and Ukrainian Carpathians (Ukr) (Seghedi et al. 2001)
are also shown for comparison. The Cãlimani low-K group (LKC) is
also highlighted. See text for discussions. Mineral phases from the
same rock are indicated by tie lines.
PETROGENESIS OF CALC-ALKALINE ROCKS: NEOGENE SUBVOLCANIC AREA (EASTERN CARPATHIANS) 89
The rocks of the medium-K series are the oldest, being em-
placed at about 10.6 Ma. Mantle-derived magma, contaminat-
ed with lower-crustal material is considered to be the source of
these rocks. The magmas had a rapid ascent toward the sur-
face, without a long-lasting stagnation period in intermediate
crustal magmatic chambers, as proven by the presence of pri-
mary garnet bearing rocks, or by the sporadic occurrence of
cognate enclaves. This is the case of Parva, Sturzii-Bucnitori,
Pleºii-Mal, Oala and Iliuþa Intrusive Units, which form small
intrusive bodies. An exception is Heniu Intrusive Unit, which
may have paused in the upper/middle crust where it experi-
enced an AEC process. Within this series, the decreasing of
the δ
18
O values as
87
Sr/
86
Sr ratios and SiO
2
increase is inter-
preted as a progressive contamination of a mantle derived
magma with a contaminant depleted in δ
18
O and enriched in
87
Sr/
86
Sr (i.e. hydrothermally altered lower crustal rocks).
The high-K series has been emplaced later in the evolution
of the magmatic activity (~9 Ma). The evolution of these mag-
mas was more complex; thus, the presence of intermediate
magma chambers needs to be considered. The magmas of the
Cornii and Valea Vinului Intrusive Units stagnated in large
chambers (see the large volume of the intrusions) where AFC
processes took place. These rocks are well crystallized, have
high K and Sr content, as well as higher
87
Sr/
86
Sr and
18
O/
16
O
ratios. The higher δ
18
O values and
87
Sr/
86
Sr ratios displayed
by Cornii and Colibiþa Intrusive Units are consistent with as-
similation of a different contaminant from that involved in
petrogenesis of the medium-K series. This could be the local
upper-crustal schists. The Mãguri Intrusive Units are the
youngest rocks in the area. They show characteristics of a hy-
drothermal system: oxygen isotope disequilibrium between
coexisting pyroxenes and amphiboles, both in host-rocks and
cognate enclaves, as well as additional mineralogical and pet-
rographical alteration effects.
Acknowledgments: Special thanks are addressed to Prof. G.
Cavarretta who made it possible that an important part of the
present study was carried out at the CNR Centro di Studio
per il Quaternario e lEvolutione Ambientale, Rome, within
the No. 52 NATO Fellowships Programme of which D.C.
Papp benefited. Laboratory managers and staff are thanked for
their help during analytical work: Prof. M. Barbieri for carry-
ing out strontium isotope analyses, A.M. Conte for the XRF
measurements, M. Serracino for technical assistance during
microprobe determinations and Prof. B. Turi for providing ac-
cess to oxygen isotope facility. M.L. Frezzotti and F. Tecce
are thanked as well for their invaluable help at various stages
of this work. The authors thank Dr. J. Lexa and Dr. M. Munte-
anu for the critical reviewing of the manuscript.
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