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 [J].

ARNETT, WD .

[3] HYDRODYNAMIC BEHAVIOR OF SUPERNOVAE EXPLOSIONS [J].

COLGATE, SA ;

WHITE, RH .

[4]

Kopal Z., 1959, Close binary systems

[5] ON OPTICAL IDENTIFICATION OF SCO X-1 [J].

SANDAGE, AR ;

OSMER, P ;

GIACCONI, R ;

GORENSTEIN, P ;

GURSKY, H ;

WATERS, J ;

BRADT, H ;

GARMIRE, G ;

SREEKANTAN, BV ;

ODA, M ;

OSAWA, K ;

JUGAKU, J .

[6] ON NATURE OF SOURCE OF X-RAY EMISSION OF SCO XR-1 [J].

SHKLOVSK.IS .