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hal.structure.identifierM2A 2019
dc.contributor.authorCASAMIQUELA, L.
hal.structure.identifierM2A 2019
dc.contributor.authorTARRICQ, Y.
hal.structure.identifierM2A 2019
dc.contributor.authorSOUBIRAN, C.
dc.date.issued2019
dc.date.conference2019-04-08
dc.description.abstractEnOpen Clusters (OCs) are excellent tracers of the formation and evolution of the Galaxy, as well as an ideal laboratory to test theories of stellar evolution. In particular, nearby OCs spanning a wide age range are commonly used as benchmark objects for galactic and stellar studies owing to the highest precision that is achievable. We have designed a project to perform an in-depth study of 45 nearby (closer than 500 pc) and old (age>300Myr) OCs. After Gaia DR2, very accurate memberships, distances, motions and ages are available for these OCs, allowing us to revise their physical properties. In particular, we are determining their chemical composition in a homogeneous way using a strictly line-by-line differential method with high-resolution, high signal-to-noise spectra, either retrieved from public archives or from our own observations. We present the first results of this project where we mesure the internal dispersions of abundances within the studied OCs and compare their chemical signatures.
dc.language.isoen
dc.title.enChemically characterising nearby evolved Open Clusters
dc.typeCommunication dans un congrès
dc.identifier.doi10.5281/zenodo.2817457
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
bordeaux.pageid.35
bordeaux.countryNL
bordeaux.conference.cityNoordwijk
bordeaux.peerReviewedoui
hal.identifierhal-02165923
hal.version1
hal.invitednon
hal.proceedingsnon
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-02165923v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2019&rft.spage=id.35&rft.epage=id.35&rft.au=CASAMIQUELA,%20L.&TARRICQ,%20Y.&SOUBIRAN,%20C.&rft.genre=unknown


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