HIGHER STABILITY LIMIT FOR NEUTRON STARS

被引：11

作者：

BOWERS, RL

GLEESON, AM

PEDIGO, RD

机构：

[1] UNIV TEXAS,CTR PARTICLE THEORY,DEPT PHYS,AUSTIN,TX 78712

[2] TEXAS A&M UNIV,DEPT PHYS,COLLEGE STN,TX

来源：

关键词：

D O I：

10.1086/154271

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：261 / 267

页数：7

共 18 条

[1] ARNETT WD, 1974, 9 U TEX ASTR PUB
[2] ARNETT WD, 1973, LATE STAGES STELLAR
[3] ARNETT WD, 1974, PREPRINT
[4] GROUND STATE OF MATTER AT HIGH DENSITIES - EQUATION OF STATE AND STELLAR MODELS
BAYM, G
PETHICK, C
SUTHERLAND, P
[J]. ASTROPHYSICAL JOURNAL, 1971, 170 (02) : 299 - +
[5] NEUTRON STAR MATTER
BAYM, G
BETHE, HA
PETHICK, CJ
[J]. NUCLEAR PHYSICS A, 1971, A175 (02) : 225 - &
[6] ROTATING NEUTRON STAR MODELS AND PULSARS
BORNER, G
COHEN, JM
[J]. ASTROPHYSICAL JOURNAL, 1973, 185 (03) : 959 - 974
[7] BOWERS RG, IN PRESS
[8] BOWERS RL, 1975, ASTROPHYS J, V196, P639, DOI 10.1086/153449
[9] EQUATION OF STATE AT ULTRAHIGH DENSITIES .1
CANUTO, V
[J]. ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1974, 12 : 167 - 214
[10] CANUTO V, IN PRESS