MICROSCOPIC INTERPRETATION OF NEUTRON STAR STRUCTURE

被引：353

作者：

ARNETT, WD

BOWERS, RL

机构：

[1] UNIV CHICAGO,ENRICO FERMI INST,CHICAGO,IL 60637

[2] NORDITA,COPENHAGEN,DENMARK

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

来源：

关键词：

D O I：

10.1086/190434

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：415 / 436

页数：22

共 56 条

[1] SUPERNOVA-REMNANTS AND PRE-SUPERNOVA MODELS
ARNETT, WD
[J]. ASTROPHYSICAL JOURNAL, 1975, 195 (03) : 727 - 733
[2] ARNETT WD, 1973, EXPLOSIVE NUCLEOSYNT
[3] ARNETT WD, 1974, LATE STAGES STELLAR
[4] ARNETT WD, 1974, NEUTRON STAR STRUCTU, V9
[5] INTERNAL STRUCTURE OF NEUTRON STARS
ARPONEN, J
[J]. NUCLEAR PHYSICS A, 1972, A191 (02) : 257 - &
[6] On super-novae
Baade, W
Zwicky, F
[J]. PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 1934, 20 : 254 - 259
[7] NEUTRON STAR MATTER
BAYM, G
BETHE, HA
PETHICK, CJ
[J]. NUCLEAR PHYSICS A, 1971, A175 (02) : 225 - &
[8] BAYM G, IN PRESS
[9] BAYM G, 1972, ASTROPHYS J, V170, P299
[10] DO OB RUNAWAYS HAVE COLLAPSED COMPANIONS
BEKENSTEIN, JD
BOWERS, RL
[J]. ASTROPHYSICAL JOURNAL, 1974, 190 (03) : 653 - 659