ON THE MAXIMUM MASS OF A UNIFORMLY ROTATING NEUTRON-STAR

被引：72

作者：

FRIEDMAN, JL ^{[1
]}

IPSER, JR ^{[1
]}

机构：

[1] UNIV FLORIDA,DEPT PHYS,GAINESVILLE,FL 32611

来源：

ASTROPHYSICAL JOURNAL | 1987年 / 314卷 / 02期

关键词：

D O I：

10.1086/165088

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

收藏

页码：594 / 597

页数：4

相关论文

共 16 条

[1] ALPAR MA, 1982, NATURE, V302, P124
[2] MICROSCOPIC INTERPRETATION OF NEUTRON STAR STRUCTURE
ARNETT, WD
BOWERS, RL
[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1977, 33 (04) : 415 - 436
[3] A MILLISECOND PULSAR
BACKER, DC
KULKARNI, SR
HEILES, C
DAVIS, MM
GOSS, WM
[J]. NATURE, 1982, 300 (5893) : 615 - 618
[4] BAYM G, 1971, AP J, V170, P307
[5] STRUCTURE AND STABILITY OF RAPIDLY ROTATING FLUID BODIES IN GENERAL RELATIVITY .1. NUMERICAL-METHOD FOR COMPUTING STRUCTURE AND ITS APPLICATION TO UNIFORMLY ROTATING HOMOGENEOUS BODIES
BUTTERWORTH, EM
IPSER, JR
[J]. ASTROPHYSICAL JOURNAL, 1976, 204 (01) : 200 - 223
[6] COMMENT ON ULTRABARIC NEUTRON STARS ARE SUPERLUMINAL
CAPORASO, G
BRECHER, K
[J]. PHYSICAL REVIEW D, 1983, 28 (10): : 2694 - 2694
[7] DO GALACTIC BULGE X-RAY SOURCES EVOLVE INTO MILLISECOND PULSARS
FABIAN, AC
PRINGLE, JE
VERBUNT, F
WADE, RA
[J]. NATURE, 1983, 301 (5897) : 222 - 223
[8] RAPIDLY ROTATING NEUTRON-STAR MODELS
FRIEDMAN, JL
IPSER, JR
PARKER, L
[J]. ASTROPHYSICAL JOURNAL, 1986, 304 (01) : 115 - 139
[9] FRIEDMAN JL, 1986, UNPUB
[10] ULTRABARIC NEUTRON STARS ARE SUPERLUMINAL
GLASS, EN
[J]. PHYSICAL REVIEW D, 1983, 28 (10): : 2693 - 2693