2016
DOI: 10.1016/j.lithos.2015.11.020
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Zircon U–Pb ages, geochemical and Sr–Nd–Pb–Hf isotopic constraints on petrogenesis of the Tarom-Olya pluton, Alborz magmatic belt, NW Iran

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Cited by 40 publications
(14 citation statements)
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“…Re gional ge ol ogy. The mag matic rocks of the AMZ are high-K calc-al ka line to al ka line (Aghazadeh et al, 2011;Asiabanha and Foden, 2012;Cas tro et al, 2013;Nabatian et al, 2016), and are tec toni cally linked to subduction of the Neo-Tethys oce anic crust be neath the Ira nian plate, and subse quent col li sion of Ara bia with Eur asia dur ing the Al pine-Hi - ma la yan orog eny that caused the for ma tion of dif fer ent orogenic belts, in clud ing the AAMB, in which oc cur such de posits as the Mazraeh-e-Shadi, Sungun, Safikhanlo, Sarilar, and oth ers (Alavi, 1994). Ce no zoic rocks of the AMZ on a Na 2 O + K 2 O ver sus SiO 2 dis crim i na tion di a gram, can be compositionally clas si fied as subalkaline ba salt, an de site/ba saltic an de site, and rhyodacite/dacite, and they plot mainly in the subalkaline field, though some of them fall into the al ka line field (Fig.…”
Section: Geological Settingmentioning
confidence: 99%
“…Re gional ge ol ogy. The mag matic rocks of the AMZ are high-K calc-al ka line to al ka line (Aghazadeh et al, 2011;Asiabanha and Foden, 2012;Cas tro et al, 2013;Nabatian et al, 2016), and are tec toni cally linked to subduction of the Neo-Tethys oce anic crust be neath the Ira nian plate, and subse quent col li sion of Ara bia with Eur asia dur ing the Al pine-Hi - ma la yan orog eny that caused the for ma tion of dif fer ent orogenic belts, in clud ing the AAMB, in which oc cur such de posits as the Mazraeh-e-Shadi, Sungun, Safikhanlo, Sarilar, and oth ers (Alavi, 1994). Ce no zoic rocks of the AMZ on a Na 2 O + K 2 O ver sus SiO 2 dis crim i na tion di a gram, can be compositionally clas si fied as subalkaline ba salt, an de site/ba saltic an de site, and rhyodacite/dacite, and they plot mainly in the subalkaline field, though some of them fall into the al ka line field (Fig.…”
Section: Geological Settingmentioning
confidence: 99%
“…The Tarom intrusions range in composition from quartz monzo-gabbro to diorite, quartz monzodiorite, monzonite, quartz monzonite, monzogranite, granodiorite, alkali granite, granite and syeno-granite (e.g., Nabatian et al 2014Nabatian et al , 2016Esmaeli et al 2015;Mehrabi et al 2016;Kouhestani et al 2017Kouhestani et al , 2018Yasami et al 2018). These I-type intrusions have high-K calc-alkaline to shoshonitic affinity and metaluminous characteristics (Irannezhadi et al 2007;Azizi et al 2009;Nabatian et al 2014Nabatian et al , 2016Yasami et al 2018) and show enrichment in Large Ion Lithophile Elements (LILE) and Light Rare Earth Elements (LREE) and negative anomalies in High Field Strength Elements (HFSE) and depletion in Heavy Rare Earth Elements (HREE) (Nabatian et al 2014(Nabatian et al , 2016Yasami et al 2018). The Tarom plutons show subduction-related arc magmatic signatures (Nabatian et al 2016).…”
Section: Introductionmentioning
confidence: 99%
“…These I-type intrusions have high-K calc-alkaline to shoshonitic affinity and metaluminous characteristics (Irannezhadi et al 2007;Azizi et al 2009;Nabatian et al 2014Nabatian et al , 2016Yasami et al 2018) and show enrichment in Large Ion Lithophile Elements (LILE) and Light Rare Earth Elements (LREE) and negative anomalies in High Field Strength Elements (HFSE) and depletion in Heavy Rare Earth Elements (HREE) (Nabatian et al 2014(Nabatian et al , 2016Yasami et al 2018). The Tarom plutons show subduction-related arc magmatic signatures (Nabatian et al 2016).…”
Section: Introductionmentioning
confidence: 99%
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“…The northwestern part of the AAMB includes two mineralized subzones named the Ahar-Arasbaran Belt (AAB) in the north and the Tarom-Hashjin metallogenic province (THMP) in the south (Figure 1) [2,3]. The THMP is known as an economically important metallogenic province in Iran [2,14,15] and includes a variety of mineral deposits such as Mn deposits, iron-skarns, manto-type Cu-Ag deposits, and Zn-Pb-Cu±Au-Ag epithermal deposits [3,[16][17][18][19]. All of these deposits are variably attributed to post-collisional magmatic processes (e.g., [20][21][22]).…”
Section: Introductionmentioning
confidence: 99%