An analysis of the distribution of globular clusters with postcollapse cores in the Galaxy

Details An analysis of the distribution of globular clusters with postcollapse cores in the Galaxy An analysis of the distribution of globular clusters with postcollapse cores in the Galaxy

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...339..904c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 339, April 15, 1989, p. 904-918. Research supported by Harvard University a

Astronomy and Astrophysics

Astrophysics

103

Astronomical Models, Distribution (Property), Globular Clusters, Gravitational Collapse, Milky Way Galaxy, Binary Stars, Brightness Distribution, Metallicity, Star Formation

Scientific paper

The structural parameters of Galactic globular clusters are studied. It is found that the distribution of post-core-collapsed clusters is much more concentrated about the Galactic center than the distribution of King (1966) clusters. A distance-independent analysis was used to address the problem of Galactic obscuration. The fact that some internal properties of clusters correlate well with global variables, such as the galactocentric radius, suggests that some external effects are important in cluster evolution.

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