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hal.structure.identifierM2A 2014
dc.contributor.authorSOUBIRAN, C.
hal.structure.identifierM2A 2014
dc.contributor.authorBLANCO-CUARESMA, S.
dc.contributor.authorHEITER, U.,
dc.date.issued2014-12
dc.date.conference2014-06-03
dc.description.abstractEnOpen clusters are key objects to study the chemical evolution of the Galactic disk, but metallicities and detailed abundances are available for only a small fraction of them. We review here the current status of metallicity determinations. Open clusters are also perfect objects to test the chemical tagging method which intends to identify stars formed from the same molecular cloud. First results about this technique are presented, based on homogeneously derived chemical abundances for a large sample of stars in open clusters.
dc.language.isoen
dc.title.enOn the chemical composition of Open Clusters
dc.typeCommunication dans un congrès
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
bordeaux.page441 - 444
bordeaux.countryFR
bordeaux.conference.cityParis
bordeaux.peerReviewedoui
hal.identifierhal-01095853
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01095853v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2014-12&rft.spage=441%20-%20444&rft.epage=441%20-%20444&rft.au=SOUBIRAN,%20C.&BLANCO-CUARESMA,%20S.&HEITER,%20U.,&rft.genre=unknown


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