Compactness of globular cluster and its evolution

Details Compactness of globular cluster and its evolution Compactness of globular cluster and its evolution

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991acaps..11..128z&link_type=abstract

(Acta Astrophysica Sinica, vol. 11, no. 2, 1991, p. 128-136) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 15, Sept.

Statistics

Computation

Computational Astrophysics, Globular Clusters, Milky Way Galaxy, Stellar Evolution, Galactic Evolution, Galactic Structure, Quantitative Analysis, Statistical Analysis

Scientific paper

The evolution of the compactness of a globular cluster is found to be closely dependent on its mass and on its position in the Galaxy. At large Galactocentric distances, the evolution is very small and is slower the larger the mass. A statistical study of the available material on the compactness shows that its distribution at smaller Galactocentric distances agrees with theoretical expectation. At large distances, the distribution is very different for different masses, possibly reflecting a close relation between the mass and condensation at the stage of formation of the cluster.

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