A SUPERLUMINOUS B-TYPE STAR IN THE LARGE MAGELLANIC CLOUD, AND ITS GALACTIC COUNTERPART

被引：27

作者：

CODE, AD

HOUCK, TE

机构：

来源：

关键词：

D O I：

10.1086/127221

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：261 / &

共 22 条

[1] Bidelman W. P., 1954, PASP, V66, P249
[2] Cannon A. J., 1901, HARVARD OBS ANN 2, V28, P177
[3] OBSERVATIONS OF EARLY-TYPE STARS IN EXTRAGALACTIC NEBULAE
CODE, AD
HOUCK, TE
[J]. ASTRONOMICAL JOURNAL, 1956, 61 (04) : 173 - 173
[4] COUSINS AWJ, 1952, OBSERVATORY, V72, P86
[5] THE DISTANCE OF THE MAGELLANIC CLOUDS
DEVAUCOULEURS, G
[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1955, 67 (398) : 350 - 354
[6] EDDINGTON AS, 1926, INTERNAL CONSTITUTIO, P16
[7] EDDINGTON AS, 1917, MNRAS, V77, P603
[8] HOUCK TE, 1956, THESIS U WISCONSIN
[9] KHOLOPOV PN, 1951, AST ZH USSR, V28, P472
[10] On the vibrational stability of gaseous stars
Ledoux, P
[J]. ASTROPHYSICAL JOURNAL, 1941, 94 (03) : 537 - 548