Merger of binary globular clusters - Case of unequal masses

Details Merger of binary globular clusters - Case of unequal masses Merger of binary globular clusters - Case of unequal masses

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.185...63m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 185, no. 1, Nov. 1991, p. 63-78. Research supported by Japan Society for t

Astronomy and Astrophysics

Astrophysics

19

Angular Momentum, Globular Clusters, Many Body Problem, Mass Transfer, Stellar Evolution, Magellanic Clouds, Mass Distribution

Scientific paper

The present study discusses the merger process of binary globular clusters for a pair of unequal-mass components. The case of mass ratio 1:0.5 is calculated by means of an N-body code with 6144 particles in total. The mass exchange between the components is found to occur through the Roche-lobe overflow. The structures of the mergers are quite similar among different cases except for the central cores which retain their initial central concentrations.

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