ON THE CONSEQUENCES OF THE GRAVOTHERMAL CATASTROPHE

被引：254
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.
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页码：483 / 498
页数：16
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