NEUTRON STAR WOBBLE IN BINARY X-RAY SOURCES

被引：48

作者：

LAMB, DQ

LAMB, FK

PINES, D

SHAHAM, J

机构：

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

[2] HEBREW UNIV,RACAH INST PHYS,JERUSALEM,ISRAEL

来源：

ASTROPHYSICAL JOURNAL | 1975年 / 198卷 / 01期

关键词：

D O I：

10.1086/181802

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

收藏

页码：L21 / L25

页数：5

相关论文

共 17 条

[1] BAYM G, TO BE PUBLISHED
[2] COMPACT X-RAY SOURCES
BLUMENTH.GR
TUCKER, WH
[J]. ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1974, 12 : 23 - 46
[3] HER-X-1 - PRECESSING BINARY PULSAR
BRECHER, K
[J]. NATURE, 1972, 239 (5371) : 325 - &
[4] GEREND D, 1974, PREPRINT
[5] GIACCONI R, 1975, 18TH P INT SOLV C
[6] NEUTRON STAR CRUSTS AND ALIGNMENT OF MAGNETIC AXES IN PULSARS
GOLDREICH, P
[J]. ASTROPHYSICAL JOURNAL, 1970, 160 (01) : L11 - +
[7] OPTICAL STUDIES OF UHURU SOURCES .4. LONG-TERM BEHAVIOR OF HZ HERCULIS = HERCULES X-1
JONES, CA
FORMAN, W
LILLER, W
[J]. ASTROPHYSICAL JOURNAL, 1973, 182 (03) : L109 - L112
[8] MODEL FOR COMPACT X-RAY SOURCES - ACCRETION BY ROTATING MAGNETIC STARS
LAMB, FK
PETHICK, CJ
PINES, D
[J]. ASTROPHYSICAL JOURNAL, 1973, 184 (01) : 271 - 289
[9] LAMB FK, 1975, 18TH P INT SOLV C
[10] LAMB FK, 1975, 7TH P TEX S REL ASTR