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hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorOLIVARES, J.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorBOUY, H.
hal.structure.identifierUniversidad Nacional de Educación a Distancia [UNED]
dc.contributor.authorSARRO, L. M.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorMIRET-ROIG, N.
hal.structure.identifierUniversidad de Cádiz = University of Cádiz [UCA]
dc.contributor.authorBERIHUETE, A.
hal.structure.identifierInstitut d'Astrophysique de Paris [IAP]
dc.contributor.authorBERTIN, E.
hal.structure.identifierCentro de Astrobiologia [Madrid] [CAB]
dc.contributor.authorBARRADO, D.
hal.structure.identifierCentro de Astrobiologia [Madrid] [CAB]
dc.contributor.authorHUÉLAMO, N.
hal.structure.identifierTokyo University of Science [Tokyo]
hal.structure.identifierNational Astronomical Observatory of Japan [NAOJ]
dc.contributor.authorTAMURA, M.
hal.structure.identifierNational Optical Astronomy Observatory [NOAO]
dc.contributor.authorALLEN, L.
hal.structure.identifierCarnegie Institution of Washington
dc.contributor.authorBELETSKY, Y.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorSERRE, S.
hal.structure.identifierDépartement d'Astrophysique (ex SAP) [DAP]
dc.contributor.authorCUILLANDRE, J.-C.
dc.date.issued2019-05
dc.identifier.issn0004-6361
dc.description.abstractEnContext. Ruprecht 147 is the oldest (2.5 Gyr) open cluster in the solar vicinity (< 300 pc), making it an important target for stellar evolution studies and exoplanet searches.Aims. We aim to derive a census of members and the luminosity, mass, and spatial distributions of the cluster.Methods. We used an astro-photometric data set including all available information from the literature together with our own observations. We processed the data with an updated version of an existent membership selection methodology.Results. We identify 259 high-probability candidate members, including 58 previously unreported. All these candidates cover the luminosity interval between G ≳ 6 mag and i ≲ 21 mag. The cluster luminosity and mass distributions are derived with an unprecedented level of details allowing us to recognize, among other features, the Wielen dip. The mass distribution in the low-mass regime drops sharply at 0.4 M⊙ even though our data are sensitive to stellar masses down to 0.1 M⊙, suggesting that most very-low-mass members left the cluster as the result of its dynamical evolution. In addition, the cluster is highly elongated (ellipticity ∼0.5) towards the galactic plane, and mass segregated.Conclusions. Our combined Gaia+DANCe data set allows us to obtain an extended list of cluster candidate members, and to derive luminosity, mass, and projected spatial distributions in the oldest open cluster of the solar vicinity.
dc.description.sponsorshipInitiative d'excellence de l'Université de Bordeaux - ANR-10-IDEX-0003
dc.language.isoen
dc.publisherEDP Sciences
dc.subject.enopen clusters and associations: individual: Ruprecht 147
dc.subject.enproper motions
dc.subject.enstars: luminosity function
dc.subject.enmass function
dc.subject.enopen clusters and associations: individual: NGC 6774
dc.title.enRuprecht 147 DANCe
dc.title.enI. Members, empirical isochrone, luminosity, and mass distributions
dc.typeArticle de revue
dc.identifier.doi10.1051/0004-6361/201834924
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
bordeaux.journalAstronomy and Astrophysics - A&A
bordeaux.pageA115
bordeaux.volume625
bordeaux.peerReviewedoui
hal.identifiercea-02137306
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//cea-02137306v1
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