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dc.contributor.authorMÄDLER, Thomas,
dc.contributor.authorJOFRÉ, Paula,
dc.contributor.authorGILMORE, Gerard,
dc.contributor.authorWORLEY, C. Clare,
hal.structure.identifierM2A 2016
dc.contributor.authorSOUBIRAN, C.
hal.structure.identifierObservatoire Astronomique de l'Université de Genève [ObsGE]
dc.contributor.authorBLANCO-CUARESMA, S.
dc.contributor.authorHAWKINS, Keith,
hal.structure.identifierFocas Research Institute
dc.contributor.authorCASEY, Andrew R.,
dc.date.issued2016
dc.identifier.issn0004-6361
dc.description.abstractEnSince the release of the Hipparcos catalog in 1997, the distance to the Pleiades open cluster has been heavily debated. The distance obtained from Hipparcos and those by alternative methods differ by 10 to 15 %. As accurate stellar distances are key to understanding stellar structure and evolution, this dilemma puts the validity of stellar evolution models into question. Using our model-independent method to determine parallaxes based on twin stars, we report individual parallaxes of 15 FGK type stars in the Pleiades in anticipation of the astrometric mission Gaia. These parallaxes give a mean cluster parallax of $7.42\pm0.09~\mathrm{mas}$ corresponding to a mean cluster distance of ${ 134.8\pm 1.7~\mathrm{pc}}$. This value agrees with the current results obtained from stellar evolution models.
dc.language.isoen
dc.publisherEDP Sciences
dc.subject.enAstrophysics - Solar and Stellar Astrophysics
dc.title.enStellar twins determine the distance of the Pleiades
dc.typeArticle de revue
dc.identifier.doi10.1051/0004-6361/201629091
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
dc.identifier.arxiv1606.03015
bordeaux.journalAstronomy and Astrophysics - A&A
bordeaux.pageid.A59
bordeaux.volume595
bordeaux.peerReviewedoui
hal.identifierhal-01358279
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01358279v1
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