A cluster analysis of young open clusters

Details A cluster analysis of young open clusters A cluster analysis of young open clusters

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64..965e&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, Sept.-Oct. 1987, p. 965-979. In Russian.

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2

Cluster Analysis, Open Clusters, Stellar Evolution, Density Distribution, Milky Way Galaxy, Radial Velocity, Stellar Color

Scientific paper

Cluster analysis methods are used to consider the galactic distribution of 224 open clusters with age up to 108years. The majority of the clusters is shown to enter condensations with characteristic dimensions of a few hundred parsecs. Some condensations, though being undistinguishable by their density from other ones, have such close values of age, integrated colour and radial velocity of their components that it is impossible to explain this by chance. It means that every such condensation is a physical entity and consists of clusters presumably connected by common origin.

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