2009/02/06 by Floor van Leeuwen · 2 citations
Physics and Astronomy · #astro-ph.GA #astro-ph.IM
paper · pdf · doi:10.1051/0004-6361/200811382
published as Astron.Astrophys.497:209-242,2009 · 34 pages, 36 figures, 7 tables. Accepted for publication by A&A
arxiv created 2009/02/06 · arxiv updated 2011/03/28
A new reduction of the astrometric data as produced by the Hipparcos mission has been published, claiming that the accuracies for nearly all stars brighter than magnitude Hp=8 are improved, by up to a factor 4, compared to the original catalogue. As correlations between the underlying abscissa residuals have also been reduced by more than an order of magnitude to an insignificant level, our ability to determine reliable parallaxes and proper motions for open clusters should be improved. The new Hipparcos astrometric catalogue is used to derive mean parallax and proper motion estimates for 20 open clusters. The HR-diagrams of the nearest clusters are compared and combined to provide future input to sets of observational isochrones. The positions of the cluster HR diagrams are consistent within different groups of clusters shown for example by the near-perfect alignment of the sequences for the Hyades and Praesepe, for Coma Ber and UMa, and for the Pleiades, NGC 2516, and Blanco 1. The groups are mutually consistent when systematic differences in Δc0 are taken into account, where the effect of these differences on the absolute magnitudes has been calibrated using field-star observations.