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.
CITATION STYLE
Diener, P., Kosovichev, A. G., Kotok, E. V., Novikov, I. D., & Pethick, C. J. (1995). Non-linear effects at tidal capture of stars by a massive black hole – II. Compressible affine models and tidal interaction after capture. Monthly Notices of the Royal Astronomical Society, 275(2), 498–506. https://doi.org/10.1093/mnras/275.2.498
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