FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1965103176> ?p ?o ?g. }

• W1965103176 endingPage "1135" @default.
• W1965103176 startingPage "1122" @default.
• W1965103176 abstract "We present detrital zircon UPb SHRIMP age patterns for the central segment (34–42°S) of an extensive accretionary complex along coastal Chile together with ages for some relevant igneous rocks. The complex consists of a basally accreted high pressure/low temperature Western Series outboard of a frontally accreted Eastern Series that was overprinted by high temperature/low pressure metamorphism. Eleven new SHRIMP detrital zircon age patterns have been obtained for meta-turbidites from the central (34–42°S) segment of the accretionary complex, four from previously undated metamorphic complexes and associated intrusive rocks from the main Andean cordillera, and three from igneous rocks in Argentina that were considered as possible sediment source areas. There are no Mesozoic detrital zircons in the accretionary rocks. Early Paleozoic zircons are an essential component of the provenance, and Grenville-age zircons and isolated grains as old as 3 Ga occur in most rocks, although much less commonly in the Western Series of the southern sector. In the northernmost sector (34–38°30′S) Proterozoic zircon grains constitute more than 50% of the detrital spectra, in contrast with less than 10% in the southern sector (39–42°S). The youngest igneous detrital zircons in both the northern Western (307 Ma) and Eastern Series (345 Ma) are considered to closely date sedimentation of the protoliths. Both oxygen and LuHf isotopic analyses of a selection of Permian to Neoproterozoic detrital zircon grains indicate that the respective igneous source rocks had significant crustal contributions. The results suggest that Early Paleozoic orogenic belts (Pampean and Famatinian) containing material recycled from cratonic areas of South America supplied detritus to this part of the paleo-Pacific coast. In contrast, in the southern exposures of the Western Series studied here, Permian detrital zircons (253–295 Ma) dominate, indicating much younger deposition. The northern sector has scarce Early to Middle Devonian detrital zircons, prominent south of 39°S. The sedimentary protolith of the northern sector was probably deposited in a passive margin setting starved of Devonian (Achalian) detritus by a topographic barrier formed by the Precordillera, and possibly Chilenia, terranes. Devonian subduction-related metamorphic and plutonic rocks developed south of 39°S, beyond the possible southern limit of Chilenia, where sedimentation of accretionary rocks continued until Permian times." @default.
• W1965103176 created "2016-06-24" @default.
• W1965103176 creator A5024081555 @default.
• W1965103176 creator A5045319666 @default.
• W1965103176 creator A5058365978 @default.
• W1965103176 creator A5063510073 @default.
• W1965103176 creator A5074416251 @default.
• W1965103176 date "2013-04-01" @default.
• W1965103176 modified "2023-10-17" @default.
• W1965103176 title "Provenance variations in the Late Paleozoic accretionary complex of central Chile as indicated by detrital zircons" @default.
• W1965103176 cites W1965954654 @default.
• W1965103176 cites W1969077651 @default.
• W1965103176 cites W1975479388 @default.
• W1965103176 cites W1984383378 @default.
• W1965103176 cites W1986642807 @default.
• W1965103176 cites W1991946360 @default.
• W1965103176 cites W1994963879 @default.
• W1965103176 cites W1998813023 @default.
• W1965103176 cites W2001396207 @default.
• W1965103176 cites W2003324046 @default.
• W1965103176 cites W2005373981 @default.
• W1965103176 cites W2007436381 @default.
• W1965103176 cites W2008608063 @default.
• W1965103176 cites W2011407246 @default.
• W1965103176 cites W2011952615 @default.
• W1965103176 cites W2013066991 @default.
• W1965103176 cites W2015488482 @default.
• W1965103176 cites W2017227039 @default.
• W1965103176 cites W2022605707 @default.
• W1965103176 cites W2025800584 @default.
• W1965103176 cites W2030457129 @default.
• W1965103176 cites W2040024714 @default.
• W1965103176 cites W2041301567 @default.
• W1965103176 cites W2043778954 @default.
• W1965103176 cites W2044175358 @default.
• W1965103176 cites W2048777742 @default.
• W1965103176 cites W2068735311 @default.
• W1965103176 cites W2077421659 @default.
• W1965103176 cites W2078165623 @default.
• W1965103176 cites W2086778250 @default.
• W1965103176 cites W2087112906 @default.
• W1965103176 cites W2088000120 @default.
• W1965103176 cites W2091229920 @default.
• W1965103176 cites W2093317589 @default.
• W1965103176 cites W2113037906 @default.
• W1965103176 cites W2135273467 @default.
• W1965103176 cites W2148917252 @default.
• W1965103176 cites W2150883528 @default.
• W1965103176 cites W2152704402 @default.
• W1965103176 cites W2161200139 @default.
• W1965103176 doi "https://doi.org/10.1016/j.gr.2012.06.016" @default.
• W1965103176 hasPublicationYear "2013" @default.
• W1965103176 type Work @default.
• W1965103176 sameAs 1965103176 @default.
• W1965103176 citedByCount "106" @default.
• W1965103176 countsByYear W19651031762013 @default.
• W1965103176 countsByYear W19651031762014 @default.
• W1965103176 countsByYear W19651031762015 @default.
• W1965103176 countsByYear W19651031762016 @default.
• W1965103176 countsByYear W19651031762017 @default.
• W1965103176 countsByYear W19651031762018 @default.
• W1965103176 countsByYear W19651031762019 @default.
• W1965103176 countsByYear W19651031762020 @default.
• W1965103176 countsByYear W19651031762021 @default.
• W1965103176 countsByYear W19651031762022 @default.
• W1965103176 countsByYear W19651031762023 @default.
• W1965103176 crossrefType "journal-article" @default.
• W1965103176 hasAuthorship W1965103176A5024081555 @default.
• W1965103176 hasAuthorship W1965103176A5045319666 @default.
• W1965103176 hasAuthorship W1965103176A5058365978 @default.
• W1965103176 hasAuthorship W1965103176A5063510073 @default.
• W1965103176 hasAuthorship W1965103176A5074416251 @default.
• W1965103176 hasBestOaLocation W19651031762 @default.
• W1965103176 hasConcept C112764850 @default.
• W1965103176 hasConcept C127313418 @default.
• W1965103176 hasConcept C13106087 @default.
• W1965103176 hasConcept C151730666 @default.
• W1965103176 hasConcept C17409809 @default.
• W1965103176 hasConcept C26687426 @default.
• W1965103176 hasConcept C2778849375 @default.
• W1965103176 hasConcept C2780049196 @default.
• W1965103176 hasConcept C42787717 @default.
• W1965103176 hasConcept C5900021 @default.
• W1965103176 hasConcept C63376196 @default.
• W1965103176 hasConcept C6494504 @default.
• W1965103176 hasConcept C77928131 @default.
• W1965103176 hasConcept C93033518 @default.
• W1965103176 hasConcept C95628711 @default.
• W1965103176 hasConceptScore W1965103176C112764850 @default.
• W1965103176 hasConceptScore W1965103176C127313418 @default.
• W1965103176 hasConceptScore W1965103176C13106087 @default.
• W1965103176 hasConceptScore W1965103176C151730666 @default.
• W1965103176 hasConceptScore W1965103176C17409809 @default.
• W1965103176 hasConceptScore W1965103176C26687426 @default.
• W1965103176 hasConceptScore W1965103176C2778849375 @default.
• W1965103176 hasConceptScore W1965103176C2780049196 @default.
• W1965103176 hasConceptScore W1965103176C42787717 @default.
• W1965103176 hasConceptScore W1965103176C5900021 @default.

• next