Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.211..263l&link_type=abstract
Astrophysics and Space Science, Volume 211, Issue 2, pp.263-275
Astronomy and Astrophysics
Astrophysics
Scientific paper
The sphere of activity which be considered in the test stars of both central galaxies and satellite galaxies is used in three-body model to study the orbital decay of interacting galaxies. It can take account of both “semi-restrictedN-body” program (Lin and Tremaine, 1983) and “multiple three-body algorithm” (Borne, 1984) at the same time. The merger time is calculated accurately. The orbital decay of satellite galaxy is characterized. Energy and angular momentum which are carried away by escaping star are computed, too.
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