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dc.contributor.authorJOFRE, P.,
dc.contributor.authorMAEDLER, T.,
dc.contributor.authorGILMORE, G.,
dc.contributor.authorCASEY, A.,
hal.structure.identifierM2A 2015
dc.contributor.authorSOUBIRAN, C.
dc.contributor.authorWORLEY, C.,
dc.date.issued2015
dc.identifier.issn0035-8711
dc.description.abstractEnDistances to stars are key to revealing a three-dimensional view of the Milky Way, yet their determination is a major challenge in astronomy. Whilst the brightest nearby stars benefit from direct parallax measurements, fainter stars are subject of indirect determinations with uncertainties exceeding 30%. We present an alternative approach to measuring distances using spectroscopically-identified twin stars. Given a star with known parallax, the distance to its twin is assumed to be directly related to the difference in their apparent magnitudes. We found 175 twin pairs from the ESO public HARPS archives and report excellent agreement with Hipparcos parallaxes within 7.5%. Most importantly, the accuracy of our results does not degrade with increasing stellar distance. With the ongoing collection of high-resolution stellar spectra, our method is well-suited to complement Gaia.
dc.language.isoen
dc.publisherOxford University Press (OUP): Policy P - Oxford Open Option A
dc.subject.enAstrophysics - Instrumentation and Methods for Astrophysics
dc.subject.enAstrophysics - Solar and Stellar Astrophysics
dc.title.enClimbing the cosmic ladder with stellar twins
dc.typeArticle de revue
dc.identifier.doi10.1093/mnras/stv1724
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
dc.identifier.arxiv1505.07806
bordeaux.journalMonthly Notices of the Royal Astronomical Society
bordeaux.page1428-1438
bordeaux.volume453
bordeaux.issue2
bordeaux.peerReviewedoui
hal.identifierhal-01158389
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01158389v1
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