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dc.contributor.authorCARRERA, R.,
dc.contributor.authorCASAMIQUELA, L.,
dc.contributor.authorBALAGUER-NÚÑEZ, L.,
dc.contributor.authorJORDI, C.,
dc.contributor.authorPANCINO, E.,
dc.contributor.authorALLENDE-PRIETO, C.,
hal.structure.identifierM2A 2014
dc.contributor.authorBLANCO-CUARESMA, S.
dc.contributor.authorMÁRTINEZ-VÁZQUEZ, C. E.,
dc.contributor.authorMURABITO, S.,
dc.contributor.authorDEL PINO, A.,
hal.structure.identifierIDIADA
dc.contributor.authorAPARICIO, A.,
dc.contributor.authorGALLART, C.,
dc.contributor.authorRECIO-BLANCO, A.,
dc.date.issued2014-12
dc.date.conference2014-09-08
dc.description.abstractEnWe present the motivation, design and current status of the Open Cluster Chemical Abundances from Spanish Observatories survey (OCCASO). Using the high resolution spectroscopic facilities available at Spanish observatories, OCCASO will derive chemical abundances in a sample of 20 to 25 open clusters older than 0.5 Gyr. This sample will be used to study in detail the formation and evolution of the Galactic disc using open clusters as tracers.
dc.language.isoen
dc.subject.enAstrophysics
dc.subject.enAstrophysics of Galaxies
dc.title.enThe Open Cluster Chemical Abundances from Spanish Observatories survey (OCCASO)
dc.typeCommunication dans un congrès
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
bordeaux.page-
bordeaux.countryES
bordeaux.conference.cityTeruel
bordeaux.peerReviewedoui
hal.identifierhal-01098170
hal.version1
hal.invitednon
hal.proceedingsoui
hal.conference.end2014-09-12
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01098170v1
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