ON THE CONSEQUENCES OF THE GRAVOTHERMAL CATASTROPHE

被引：247

作者：

LYNDENBELL, D

EGGLETON, PP

机构：

[1] Institute ofAstronomy, Observatories, Cambridge,CE3 OHA, United Kingdom

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1980年 / 191卷 / 02期

关键词：

Astrophysics - Eigenvalues and eigenfunctions - NASA;

D O I：

10.1093/mnras/191.3.483

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The cores of globular clusters evolve independently of the outer parts and eventually achieve a self-similar evolution with a shrinking almost isothermal portion followed by a power law density profile, p 0: r-O:. It is proved that a is in the range 2 © Royal Astronomical Society • Provided by the NASA Astrophysics Data System.

引用

页码：483 / 498

页数：16

共 28 条

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[2] AARSETH SJ, 1974, ASTRON ASTROPHYS, V35, P237
[3] AARSETH SJ, 1972, ASTRON ASTROPHYS, V21, P255
[4] NUMERICAL EXPERIMENTS ON N-BODY PROBLEM
AARSETH, SJ
[J]. ASTROPHYSICS AND SPACE SCIENCE, 1971, 14 (01) : 20 - &
[5] ANTONOV VA, 1962, 7 LEN STAT U B, P135
[6] EVOLUTION OF LOW MASS STARS
EGGLETON, PP
[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1971, 151 (03) : 351 - &
[7] HENON M, 1975, IAU69 S, P134
[8] Henon M., 1973, DYNAMICAL STRUCTURE, P183
[9] Henon M., 1960, ANN DASTROPHYSIQUE, V23, P668
[10] HENON M, 1971, ASTROPHYS SPACE SCI, V14, P751

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