Moving Star Clusters in the Solar Neighborhood (Orlov+, 1995)

Details Moving Star Clusters in the Solar Neighborhood (Orlov+, 1995) Moving Star Clusters in the Solar Neighborhood (Orlov+, 1995)

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ycat..80720495o&link_type=abstract

VizieR On-line Data Catalog: J/AZh/72/495. Originally published in: 1995AZh....72..495O

Physics

Associations: Stellar, Space Velocities

Scientific paper

Two cluster analysis algorithms - the principal stars method and the hierarchical clustering method - are used to identify moving star clusters in a sample of 1947 single and multiple stars in the nearby solar neighborhood with known space velocities from the Gliese and Jahreiss (Cat. ) catalog. Five rich moving clusters containing from 35 to 40 stars with velocities differing by not more than 6 km/s from the centroid value have been reliably identified. In addition, seven poor clusters have been identified with less confidence. Rich moving clusters include about 10% of all stars with known space velocities. (6 data files).

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