J/A+A/598/A48ivo://CDS.VizieR/J/A+A/598/A48doi:10.26093/cds/vizier.35980048CDSGalli P.A.B.Moraux E.Bouy H.Bouvier J.Olivares J.Teixeira R.2019-05-02T09:13:25Z2017-01-31T12:57:09ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.fropen-star-clustersproper-motionsstellar-distanceThe distance to the Pleiades open cluster has been extensively debated in the literature over several decades. Although different methods point to a discrepancy in the trigonometric parallaxes produced by the Hipparcos mission, the number of individual stars with known distances is still small compared to the number of cluster members to help solve this problem. We provide a new distance estimate for the Pleiades based on the moving cluster method, which will be useful to further discuss the so-called Pleiades distance controversy and compare it with the very precise parallaxes from the Gaia space mission. We apply a refurbished implementation of the convergent point search method to an updated census of Pleiades stars to calculate the convergent point position of the cluster from stellar proper motions. Then, we derive individual parallaxes for 64 cluster members using radial velocities compiled from the literature, and approximate parallaxes for another 1146 stars based on the spatial velocity of the cluster. This represents the largest sample of Pleiades stars with individual distances to date. The parallaxes derived in this work are in good agreement with previous results obtained in different studies (excluding Hipparcos) for individual stars in the cluster. We report a mean parallax of 7.44+/-0.08mas and distance of 134.4^+2.9^_-2.8_pc that is consistent with the weighted mean of 135.0+/-0.6pc obtained from the non-Hipparcos results in the literature. Our result for the distance to the Pleiades open cluster is not consistent with the Hipparcos catalog, but favors the recent and more precise distance determination of 136.2+/-1.2pc pc obtained from Very Long Baseline Interferometry observations. It is also in good agreement with the mean distance of 133+/-5pc obtained from the first trigonometric parallaxes delivered by the Gaia satellite for the brightest cluster members in common with our sample.2017A&A...598A..48Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/598/A48CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/563/A45 : Pleiades cluster membership probabilities (Sarro+, 2014)J/A+A/577/A148 : The Seven Sisters DANCe. I. Pleiades (Bouy+, 2015)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/598/A48https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/598/A48http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/598/A48https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/598/A48https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/598/A48http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/598/A48GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/598/A48/table4 (Approximate parallaxes for 1146 stars)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/598/A48/table4?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/598/A48/table4?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/598/A48/table4?GETtext/xml+votable180.050000true51.866416724.08301110.0055555555555555564/28-29 5/90-91 94 120-121 123-124 126-127 6/355 358-359 380 382-383 405 407 413-414 437 439 488-489 491 500 502-503 836-837 848-849 1066 1152-1153 1160 1162 1184-1186 1193-1194https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/598/A48?format=asciidefaultJ/A+A/598/A48/table4Approximate parallaxes for 1146 starsSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintDANCeDANCe Survey ID (JHHMMSS.ss+DDMMSS.s)meta.id;meta.maincharRAJ2000Right Ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainpmRAProper motion in RA (pmRA*cos(DE))mas/yrpos.pm;pos.eq.rafloate_pmRAError on proper motion in RAmas/yrstat.error;pos.pm;pos.eq.rafloatpmDEProper motion in DEmas/yrpos.pm;pos.eq.decfloate_pmDEError on proper motion in DEmas/yrstat.error;pos.pm;pos.eq.decfloatplxKinematic parallaxmaspos.parallax.dynfloate_plxError on kinematic parallaxmasstat.error;pos.parallaxfloat