NONLINEAR EFFECTS AT TIDAL CAPTURE OF STARS BY A MASSIVE BLACK-HOLE .2. COMPRESSIBLE AFFINE MODELS AND TIDAL INTERACTION AFTER CAPTURE

被引：25

作者：

DIENER, P

KOSOVICHEV, AG

KOTOK, EV

NOVIKOV, ID

PETHICK, CJ

机构：

[1] THEORET ASTROPHYS CTR,DK-2100 COPENHAGEN O,DENMARK

[2] STANFORD UNIV,HEPL,CTR ASTROPHYS & SPACE SCI,STANFORD,CA 94305

[3] UNIV CAMBRIDGE,INST ASTRON,CAMBRIDGE CB3 0HA,ENGLAND

[4] CRIMEAN ASTROPHYS OBSERV,NAUCHNYI 334413,UKRAINE

[5] MV KELDYSH APPL MATH INST,MOSCOW 125047,RUSSIA

[6] NORDITA,DK-2100 COPENHAGEN O,DENMARK

[7] PN LEBEDEV PHYS INST,CTR ASTRO SPACE,MOSCOW 117810,RUSSIA

[8] UNIV ILLINOIS,DEPT PHYS,URBANA,IL 61801

[9] UNIV WASHINGTON,INST NUCL THEORY,SEATTLE,WA 98195

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1995年 / 275卷 / 02期

关键词：

BLACK HOLE PHYSICS; CELESTIAL MECHANICS; STELLAR DYNAMICS; GALAXIES; NUCLEI;

D O I：

10.1093/mnras/275.2.498

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 and 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.

引用

页码：498 / 506

页数：9

共 24 条

[1] MECHANICS OF THE AFFINE STAR MODEL [J].