MODELS FOR RAPIDLY ROTATING PRE-MAIN SEQUENCE STARS

被引：6

作者：

MOSS, DL ^{[1
]}

机构：

[1] MANCHESTER UNIV,DEPT MATH,MANCHESTER M13 9PL,LANCASHIRE,ENGLAND

来源：

关键词：

D O I：

10.1093/mnras/161.3.225

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：225 / 337

页数：113

共 15 条

[1]

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[2]

EZER D, 1966, COLLOQUIUM LATE TYPE

[3] UNIFORMLY ROTATING MAIN-SEQUENCE STARS [J].

FAULKNER, J ;

ROXBURGH, IW ;

STRITTMATTER, PA .

[4]

Hayashi C., 1961, PUBLICATION ASTRONOM, V13, P450

[5] STELLAR EVOLUTION .I. APPROACH TO MAIN SEQUENCE [J].

IBEN, I .

[6] STRUCTURE + STABILITY OF ROTATING GAS MASSES [J].

JAMES, RA .

[7]

Kippenhahn R., 1970, STELLAR ROTATION

[8]

KRAFT RP, 1967, ASTROPHYS J, V135, P748

[9]

Kumar S. S., 1969, LOW LUMINOSITY STARS

[10]

LUCY LB, 1967, Z ASTROPHYS, V65, P89