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dc.contributor.authorFreville, K.
dc.contributor.authorCenki-Tok, B.
dc.contributor.authorTrap, P.
dc.contributor.authorRabin, M.
dc.contributor.authorLeyreloup, A.
dc.contributor.authorRegnier, Jean-Luc
dc.contributor.authorWhitney, D. L.
dc.date.accessioned2020-11-20T15:02:20Z
dc.date.available2020-11-20T15:02:20Z
dc.date.issued2016
dc.identifier.issn0263-4929
dc.identifier.issn1525-1314
dc.identifier.urihttps://doi.org/10.1111/jmg.12188
dc.identifier.urihttps://hdl.handle.net/20.500.12809/2471
dc.descriptionWOS: 000379933100003en_US
dc.description.abstractThis paper aims to decipher the thermal evolution of the Montagne Noire Axial Zone (MNAZ, southern French Massif Central) gneiss core and its metasedimentary cover through determination of P-T paths and temperature gradients. Migmatitic gneiss from the core of the dome record a clockwise evolution culminating at 725 +/- 25 degrees C and 0.8 +/- 0.1 GPa with partial melting, followed by a decompression path with only minor cooling to 690 +/- 25 degrees C and 0.4 +/- 0.1 GPa. Field structural analyses as well as detailed petrological observations indicate that the cover sequence experienced LP-HT metamorphism. Apparent thermal gradients within the cover were determined with garnet-biotite thermometry and Raman Spectroscopy on Carbonaceous Matter. High-temperature apparent gradients (e.g. similar to 530 degrees C km(-1) along one transect) are explained by late brittle-ductile extensional shearing evidenced by phyllonites that post-date peak metamorphism. In areas where normal faults are less abundant and closely spaced, gradients of similar to 20 to 50 degrees C km(-1) are calculated. These gradients can be accounted for by a combination of dome emplacement and ductile shearing (collapse of isotherms), without additional heat input. Finally, the thermal evolution of the MNAZ is typical for many gneiss domes worldwide as well as with other LP-HT terranes in the Variscides.en_US
dc.description.sponsorshipINSU/SYSTER; US NSFNational Science Foundation (NSF) [EAR-1050020]; Directorate For GeosciencesNational Science Foundation (NSF)NSF - Directorate for Geosciences (GEO) [1050020] Funding Source: National Science Foundationen_US
dc.description.sponsorshipThis project was funded by a INSU/SYSTER program granted to B. Cenki-Tok. Additional support was provided by US NSF grant EAR-1050020 to Ch. Teyssier and D.L. Whitney. K. Freville thanks O. Beyssac for assistance during RSCM analysis. We thank the support of the Microsonde Sud equipment. A. Leyreloup and J.-L. Regnier thank the bachelor and master students of the University of Montpellier 2 who participated to the mapping of isograds in the eastern termination of the dome. The manuscript benefited from constructive reviews from R. Palin and an anonymous reviewer. M. Brown is thanked for editorial handling.en_US
dc.item-language.isoengen_US
dc.publisherWileyen_US
dc.item-rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectGneiss Domeen_US
dc.subjectMontagne Noireen_US
dc.subjectP-T Evolutionen_US
dc.subjectThermal Gradientsen_US
dc.titleThermal interaction of middle and upper crust during gneiss dome formation: example from the Montagne Noire (French Massif Central)en_US
dc.item-typearticleen_US
dc.contributor.departmentMÜ, Mühendislik Fakültesi, Jeoloji Mühendisliği Bölümüen_US
dc.contributor.authorID0000-0002-5398-1880
dc.contributor.institutionauthorRegnier, Jean-Luc
dc.identifier.doi10.1111/jmg.12188
dc.identifier.volume34en_US
dc.identifier.issue5en_US
dc.identifier.startpage447en_US
dc.identifier.endpage462en_US
dc.relation.journalJournal of Metamorphic Geologyen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US


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