Red giants in open clusters - XIV. Mean radial velocities for 1309 stars and 166 open clusters

Mermilliod, J. C.Mayor, M.Udry, S.2010-11-302010-11-302010-11-30200810.1051/0004-6361:200809664https://infoscience.epfl.ch/handle/20.500.14299/61310WOS:000256690600032Context. Radial velocities have proved to be an efficient method for membership determination if there are at least 2 or 3 red giants in a cluster. They are necessary for galactic studies, but are still missing for many open clusters.galaxy : open clusters and associations : generaltechniques : radial velocitiesstars : late-type10 Spectroscopic BinariesOld Open ClustersCoravel ObservationsStellar EvolutionNgc 752MembershipMetallicityPhotometryNgc-2360CatalogRed giants in open clusters - XIV. Mean radial velocities for 1309 stars and 166 open clusterstext::journal::journal article::research article