Physics
Scientific paper
Jul 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.275..498d&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 275, Issue 2, pp. 498-506.
Physics
10
Black Hole Physics, Celestial Mechanics, Stellar Dynamics, Galaxies: Nuclei
Scientific paper
This paper continues our investigations published in Paper I. The tidal interaction of stars with a massive black hole after tidal capture is investigated in the framework of the ellipsoidal `affine' stellar model proposed by Carter & Luminet. We investigate the influence of the orientation of the ellipsoidal stellar model and the influence of the phase and amplitude of the oscillations on the subsequent passages. Finally a parametrization of the probability for a star to lose (or gain) energy during subsequent passages is found for a compressible model.
Diener Peter
Kosovichev Aleksandr G.
Kotok E. V.
Novikov Igor D.
Pethick Christopher J.
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