Open clusters proper motions based on UCAC2

DOI

We present the kinematics of hundreds of open clusters, based on the UCAC2 Catalogue positions and proper motions. Membership probabilities were obtained for the stars in the cluster fields by applying a statistical method uses stellar proper motions. All open clusters with known distance were investigated, and for 75 clusters this is the first determination of the mean proper motion. The results, including the DSS images of the cluster's fields with the kinematic members marked, are incorporated in the Open Clusters Catalogue supported on line by our group.

Cone search capability for table J/A+A/446/949/pm (Stars from all 430 clusters)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34460949
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/446/949
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/446/949
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/446/949
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/446/949
Provenance
Creator Dias W.S.; Florio; V.; Assafin M.; Alessi B.S.; Libero V.
Publisher CDS
Publication Year 2006
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Natural Sciences; Physics; Stellar Astronomy