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dc.contributor.authorMoyano-Cambero, Carles E.
dc.contributor.authorTrigo-Rodríguez, Josep M.
dc.contributor.authorBenito, M. Isabel
dc.contributor.authorAlonso-Azcárate, Jacinto
dc.contributor.authorLee, Martin R.
dc.contributor.authorMestres, Narcís.
dc.contributor.authorMartínez-Jiménez, Marina
dc.contributor.authorMartín-Torres, Francisco J.
dc.contributor.authorFraxedas, Jordi
dc.date.accessioned2020-05-01T12:45:01Z
dc.date.available2020-05-01T12:45:01Z
dc.date.issued2017-06
dc.identifier.citationMoyano-Cambero , C E , Trigo-Rodríguez , J M , Benito , M I , Alonso-Azcárate , J , Lee , M R , Mestres , N , Martínez-Jiménez , M , Martín-Torres , F J & Fraxedas , J 2017 , ' Petrographic and geochemical evidence for multiphase formation of carbonates in the Martian orthopyroxenite Allan Hills 84001 ' , Meteoritics and Planetary Science , vol. 52 , no. 6 , pp. 1030-1047 . https://doi.org/10.1111/maps.12851en
dc.identifier.issn1086-9379
dc.identifier.otherPURE: 160230886
dc.identifier.otherPURE UUID: ae52b0c7-8a16-4c4a-ae0f-125dd38260fb
dc.identifier.otherRIS: urn:E5B98C6241CD96EC436EF54A5E546E06
dc.identifier.otherScopus: 85015057628
dc.identifier.otherRIS: urn:5F62B751D30BF2AE255768667ACA0D38
dc.identifier.otherORCID: /0000-0001-6479-2236/work/73482909
dc.identifier.urihttps://hdl.handle.net/2164/14223
dc.descriptionThis research has been funded by the Spanish Ministry of Science and Innovation (projects: AYA2011‐26,522, AYA 2015‐67175‐P, CTQ2015‐62,635‐ERC, and CTQ2014‐60,119‐P to which J.M. Trigo‐Rodríguez and C.E. Moyano‐Cambero acknowledge financial support). The UK Science and Technology Facilities Council is also thanked for funding through grants ST/H002960/1, ST/K000942/1, and ST/L002167/1. ICN2 and ICMAB acknowledge support of the Spanish MINECO through the Severo Ochoa Centers of Excellence Program under Grants SEV‐2013‐0295 and SEV‐2015‐0496, respectively. We acknowledge B. Ballesteros and M. Rosado from the ICN2 Electron Microscopy Division, and A. Fernández from the ICTS (National Center of Electronic Microscopy) for the SEM, EDS, and microprobe measurements. We also thank the NASA Meteorite Working Group, and the Johnson Space Center for providing the ALH 84001,82 section. This study was done in the frame of a PhD on Physics at the Autonomous University of Barcelona (UAB) under the direction of J. M. Trigo‐Rodríguez.en
dc.format.extent18
dc.language.isoeng
dc.relation.ispartofMeteoritics and Planetary Scienceen
dc.rights© 2017 The Authors. Meteoritics & Planetary Science 1030 published by Wiley Periodicals, Inc. on behalf of The Meteoritical Society. This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited. https://creativecommons.org/licenses/by/4.0/en
dc.subjectAstrophysics - Earth and Planetary Astrophysicsen
dc.subjectPetrographicen
dc.subjectgeochemical evidenceen
dc.subjectMarsen
dc.subjectQE Geologyen
dc.subjectQB Astronomyen
dc.subjectOtheren
dc.subjectST/H002960/1en
dc.subjectST/K000942/1en
dc.subjectST/L002167/1en
dc.subjectSupplementary Dataen
dc.subject.lccQEen
dc.subject.lccQBen
dc.titlePetrographic and geochemical evidence for multiphase formation of carbonates in the Martian orthopyroxenite Allan Hills 84001en
dc.typeJournal articleen
dc.contributor.institutionUniversity of Aberdeen.Geology and Geophysicsen
dc.description.statusPeer revieweden
dc.description.versionPublisher PDFen
dc.identifier.doihttps://doi.org/10.1111/maps.12851
dc.identifier.urlhttp://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-62454en
dc.identifier.urlhttps://ui.adsabs.harvard.edu/abs/2017M&PS...52.1030Men


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