2013
DOI: 10.1016/j.tecto.2012.12.032
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Reconstruction of the Early Ordovician Famatinian arc through thermobarometry in lower and middle crustal exposures, Sierra de Valle Fértil, Argentina

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Cited by 45 publications
(39 citation statements)
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References 61 publications
(110 reference statements)
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“…Consequently, metamorphic conditions of the Cerro Olivo Complex [Lenz et al, 2011] could be explained by arc-related high-grade metamorphism and magmatism followed by the accretion of the Nico Pérez Terrane and the Río de la Plata Craton (Figures 8a and 8b). Similar P-T conditions in arc settings were reported by Tibaldi et al [2013] and Maki et al [2014] in the Famatinian arc (western Sierras Pampeanas) and the Higo metamorphic terrane (central Kyushu), respectively. Likewise, Basei et al [2011a] interpreted a collisional event at 635 ± 10 Ma in the Cerro Olivo Complex.…”
Section: Implications For Western Gondwanasupporting
confidence: 75%
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“…Consequently, metamorphic conditions of the Cerro Olivo Complex [Lenz et al, 2011] could be explained by arc-related high-grade metamorphism and magmatism followed by the accretion of the Nico Pérez Terrane and the Río de la Plata Craton (Figures 8a and 8b). Similar P-T conditions in arc settings were reported by Tibaldi et al [2013] and Maki et al [2014] in the Famatinian arc (western Sierras Pampeanas) and the Higo metamorphic terrane (central Kyushu), respectively. Likewise, Basei et al [2011a] interpreted a collisional event at 635 ± 10 Ma in the Cerro Olivo Complex.…”
Section: Implications For Western Gondwanasupporting
confidence: 75%
“…Similar P‐T conditions in arc settings were reported by Tibaldi et al . [] and Maki et al . [] in the Famatinian arc (western Sierras Pampeanas) and the Higo metamorphic terrane (central Kyushu), respectively.…”
Section: Discussionmentioning
confidence: 99%
“…(source data: Tulloch and Challis 44 ; Eberhart-Phillips and Reyners 45 ; Scott, et al 29 ; De Paoli et al 47 . Figure adapted from Tibaldi et al 77 ). ( B ) Schematic cross section of Cordillera Zealandia showing the inferred under-thrust Gondwana margin converted to an eclogitic root following partial melting during a flare-up event, which produced the voluminous WFO and SPS suite magmatism. …”
Section: Crustal Profilementioning
confidence: 99%
“…Peak granulite facies metamorphism is spatially associated with the Famatina arc, but different crustal levels are exposed on either side of the Valle Fertil lineament. Andalusite and sillimanite bearing pelitic protoliths east of the Valle Fertil Lineament experienced migmatization (Figure ) at ∼750–900°C at ∼5–7 kbar via the intrusion of mafic and intermediate melts during construction of the Famatina arc [e.g., Hauzenberger et al , ; Büttner et al , ; Murra and Baldo , ; Delpino et al , ; Castro de Machuca et al , ; Otamendi et al , ; Gallien et al , ; Tibaldi et al , ; Larrovere et al , ; Otamendi et al , ; Tibaldi et al , ] and preserve counterclockwise pressure‐temperature paths and near isobaric cooling from peak temperatures [e.g., Hauzenberger et al , ; Delpino et al , ; Otamendi et al , ; Gallien et al , ]. Migmatization occurred at ∼465 Ma, although ages from multiple systems within the high‐grade rocks range from ∼470 to 402 Ma [e.g., Hauzenberger et al , ; Hockenreiner et al , ; Lucassen and Becchio , ; Galindo et al , ; Porcher et al , ; Büttner et al , ; Steenken et al , ; Castro de Machuca et al , ; Steenken et al , ; Gallien et al , ; Varela et al , ] and have been interpreted as cooling from peak conditions or as distinct metamorphic and deformation events.…”
Section: Introductionmentioning
confidence: 99%