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dc.contributor.authorCANTAT-GAUDIN, T.
dc.contributor.authorVALLENARI, A.
dc.contributor.authorSORDO, R.
dc.contributor.authorPENSABENE, F.
dc.contributor.authorKRONE-MARTINS, A.
hal.structure.identifierUniversidade de Lisboa = University of Lisbon = Université de Lisbonne [ULISBOA]
dc.contributor.authorMOITINHO, A.
dc.contributor.authorJORDI, C.
dc.contributor.authorCASAMIQUELA, L.
hal.structure.identifierUniversitat de Barcelona [UB]
dc.contributor.authorBALAGUER-NÚÑEZ, L.
hal.structure.identifierM2A 2018
dc.contributor.authorSOUBIRAN, C.
hal.structure.identifierFORMATION STELLAIRE 2018
dc.contributor.authorBROUILLET, N.
dc.date.issued2018
dc.identifier.issn0004-6361
dc.description.abstractEnThe Tycho-Gaia Astrometric Solution (TGAS) subset of the first Gaia catalogue contains an unprecedented sample of proper motions and parallaxes for two million stars brighter than G~12 mag. We take advantage of the full astrometric solution available for those stars to identify the members of known open clusters and compute mean cluster parameters using either TGAS or UCAC4 proper motions, and TGAS parallaxes. We apply an unsupervised membership assignment procedure to select high probability cluster members, we use a Bayesian/MCMC technique to fit stellar isochrones to the observed 2MASS JHK$_s$ magnitudes of the member stars and derive cluster parameters (age, metallicity, extinction, distance modulus), and we combine TGAS data with spectroscopic radial velocities to compute full Galactic orbits. We obtain mean astrometric parameters (proper motions and parallaxes) for 128 clusters closer than about 2 kpc, and cluster parameters from isochrone fitting for 26 of them located inside 1 kpc from the Sun. We show the orbital parameters obtained from integrating 36 orbits in a Galactic potential.
dc.language.isoen
dc.publisherEDP Sciences
dc.rights.urihttp://creativecommons.org/licenses/by/
dc.subject.enAstrophysics - Astrophysics of Galaxies
dc.title.enCharacterising Open Clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution
dc.typeArticle de revue
dc.identifier.doi10.1051/0004-6361/201731251
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
dc.identifier.arxiv1801.10042
bordeaux.journalAstronomy and Astrophysics - A&A
bordeaux.pageid.A49
bordeaux.volume615
bordeaux.peerReviewedoui
hal.identifierhal-01729110
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01729110v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Astronomy%20and%20Astrophysics%20-%20A&A&rft.date=2018&rft.volume=615&rft.spage=id.A49&rft.epage=id.A49&rft.eissn=0004-6361&rft.issn=0004-6361&rft.au=CANTAT-GAUDIN,%20T.&VALLENARI,%20A.&SORDO,%20R.&PENSABENE,%20F.&KRONE-MARTINS,%20A.&rft.genre=article


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