COMMENTS ON SHKLOVSKYS MODEL FOR X-RAY SOURCE SCO XR-1

被引：20

作者：

SOFIA, S

机构：

来源：

关键词：

D O I：

10.1086/180056

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L59 / &

共 6 条

[1] Arnett W.D., 1967, Canadian Journal of Physics, V45, P1621
[2] GRAVITATIONAL COLLAPSE AND WEAK INTERACTIONS
ARNETT, WD
[J]. CANADIAN JOURNAL OF PHYSICS, 1966, 44 (11) : 2553 - +
[3] HYDRODYNAMIC BEHAVIOR OF SUPERNOVAE EXPLOSIONS
COLGATE, SA
WHITE, RH
[J]. ASTROPHYSICAL JOURNAL, 1966, 143 (03) : 626 - &
[4] Kopal Z., 1959, Close binary systems
[5] ON OPTICAL IDENTIFICATION OF SCO X-1
SANDAGE, AR
OSMER, P
GIACCONI, R
GORENSTEIN, P
GURSKY, H
WATERS, J
BRADT, H
GARMIRE, G
SREEKANTAN, BV
ODA, M
OSAWA, K
JUGAKU, J
[J]. ASTROPHYSICAL JOURNAL, 1966, 146 (01) : 316 - +
[6] ON NATURE OF SOURCE OF X-RAY EMISSION OF SCO XR-1
SHKLOVSK.IS
[J]. ASTROPHYSICAL JOURNAL, 1967, 148 (1P2) : L1 - &