RELATIVISTIC, SPHERICALLY SYMMETRIC STAR CLUSTERS .3. STABILITY OF COMPACT ISOTROPIC MODELS

被引:74
作者
IPSER, JR
机构
关键词
D O I
10.1086/150169
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:17 / +
页数:1
相关论文
共 13 条
[1]  
Eddington A. S, 1916, MNRAS, V76, P572, DOI [10.1093/mnras/76.7.572, DOI 10.1093/MNRAS/76.7.572]
[2]   RELATIVISTIC STELLAR DYNAMICS [J].
FACKERELL, ED .
ASTROPHYSICAL JOURNAL, 1968, 153 (2P1) :643-+
[3]  
FACKERELL ED, UNPUBLISHED
[4]  
FACKERELL ED, 1966, THESIS U SYDNEY
[5]  
FACKERELL ED, IN PRESS
[6]   GRAVITATIONAL RED-SHIFTS IN QUASI-STELLAR OBJECTS [J].
HOYLE, F ;
FOWLER, WA .
NATURE, 1967, 213 (5074) :373-&
[7]   RELATIVISTIC SPHERICALLY SYMMETRIC STAR CLUSTERS .I. STABILITY THEORY FOR RADIAL PERTURBATIONS [J].
IPSER, JR ;
THORNE, KS .
ASTROPHYSICAL JOURNAL, 1968, 154 (1P1) :251-+
[9]   NORMAL MODES OF RADIAL PULSATION OF STARS AT END POINT OF THERMONUCLEAR EVOLUTION [J].
MELTZER, DW ;
THORNE, KS .
ASTROPHYSICAL JOURNAL, 1966, 145 (02) :514-+
[10]  
THORNE KS, 1967, HIGH ENERGY ASTROPHY, V3