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dc.rights.license© C. Reylé et al. 2021es
dc.contributor.authorReylé, C.-
dc.contributor.authorJardine, K.-
dc.contributor.authorFouqué, P.-
dc.contributor.authorCaballero, J. A.-
dc.contributor.authorSmart, R. L.-
dc.contributor.authorSozzetti, A.-
dc.date.accessioned2022-04-11T11:10:53Z-
dc.date.available2022-04-11T11:10:53Z-
dc.date.issued2021-06-30-
dc.identifier.citationAstronomy and Astrophysics 650: A201(2021)es
dc.identifier.issn0004-6361-
dc.identifier.otherhttps://www.aanda.org/articles/aa/full_html/2021/06/aa40985-21/aa40985-21.html-
dc.identifier.urihttp://hdl.handle.net/20.500.12666/732-
dc.descriptionThe animation and a zoomable version of Fig. B.1 are available at https://www.aanda.org Table A.1 is only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/cat/J/A+A/650/A201, at https://gruze.org/10pc/, and at https://gucds.inaf.it/es
dc.description.abstractContext. The nearest stars provide a fundamental constraint for our understanding of stellar physics and the Galaxy. The nearby sample serves as an anchor where all objects can be seen and understood with precise data. This work is triggered by the most recent data release of the astrometric space mission Gaia and uses its unprecedented high precision parallax measurements to review the census of objects within 10 pc. Aims. The first aim of this work was to compile all stars and brown dwarfs within 10 pc observable by Gaia and compare it with the Gaia Catalogue of Nearby Stars as a quality assurance test. We complement the list to get a full 10 pc census, including bright stars, brown dwarfs, and exoplanets. Methods. We started our compilation from a query on all objects with a parallax larger than 100 mas using the Set of Identifications, Measurements, and Bibliography for Astronomical Data database (SIMBAD). We completed the census by adding companions, brown dwarfs with recent parallax measurements not in SIMBAD yet, and vetted exoplanets. The compilation combines astrometry and photometry from the recent Gaia Early Data Release 3 with literature magnitudes, spectral types, and line-of-sight velocities. Results. We give a description of the astrophysical content of the 10 pc sample. We find a multiplicity frequency of around 27%. Among the stars and brown dwarfs, we estimate that around 61% are M stars and more than half of the M stars are within the range from M3.0 V to M5.0 V. We give an overview of the brown dwarfs and exoplanets that should be detected in the next Gaia data releases along with future developments. Conclusions. We provide a catalogue of 540 stars, brown dwarfs, and exoplanets in 339 systems, within 10 pc from the Sun. This list is as volume-complete as possible from current knowledge and it provides benchmark stars that can be used, for instance, to define calibration samples and to test the quality of the forthcoming Gaia releases. It also has a strong outreach potential.es
dc.description.sponsorshipThe authors thank the referee for useful and prompt comments. C.R. thanks Catherine Turon for fruitful discussions on the parallax measurements across the history. C.R. thanks Will J. Cooper for his contribution to plotting. This work was supported by the “Programme National de Physique Stellaire” (PNPS) of CNRS/INSU co-funded by CEA and CNES. R.L.S. and A.S. acknowledge support from the Italian Space Agency (ASI) under contract 2018-24-HH.0. A.S. acknowledges the financial contribution from the agreement ASI-INAF n.2018-16-HH.0. J.A.C. acknowledges financial support from the Agencia Estatal de Investigación of the Ministerio de Ciencia, Innovación y Universidades and the ERDF through project PID2019-109522GB-C51/AEI/10.13039/501100011033. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. This research has made use of the NASA Exoplanet Archive, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program. This research has made use of data obtained from or tools provided by the portal exoplanet.eu of The Extrasolar Planets Encyclopædia. This research has made use of the Washington Double Star Catalog maintained at the U.S. Naval Observatory. This research has made use of the TOPCAT (http://www.starlink.ac.uk/topcat/) tool (Taylor et al. 2005).es
dc.language.isoenges
dc.publisherEDP Scienceses
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-109522GB-C51/ES/ENANAS MARRONES Y PLANETAS AISLADOS Y ALREDEDOR DE ESTRELLAS/-
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internationales
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/-
dc.subjectParallaxeses
dc.subjectStars: late typees
dc.subjectPlanetary systemses
dc.subjectSolar neighborhoodes
dc.subjectGalaxies: stellar contentes
dc.subjectCatalogses
dc.titleThe 10 parsec sample in the Gaia eraes
dc.typeinfo:eu-repo/semantics/articlees
dc.contributor.orcidReylé, C. [0000-0003-2258-2403]-
dc.contributor.orcidJardine, K. [0000-0001-6068-2734]-
dc.contributor.orcidFouqué, P. [0000-0002-1436-7351]-
dc.contributor.orcidCaballero, J. A. [0000-0002-7349-1387]-
dc.contributor.orcidSozzetti, A. [0000-0002-7504-365X]-
dc.identifier.doi10.1051/0004-6361/202140985-
dc.identifier.e-issn1432-0746-
dc.contributor.funderAgencia Estatal de Investigación (AEI)-
dc.contributor.funderAgenzia Spaziale Italiana (ASI)-
dc.contributor.funderIstituto Nazionale di Astrofisica (INAF)-
dc.description.peerreviewedPeerreviewes
dc.identifier.funderhttp://dx.doi.org/10.13039/501100011033-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003981-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100005184-
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501-
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