INFLUENCE OF ROTATION ON MAXIMUM MASS OF PULSATIONALLY STABLE STARS

被引：16

作者：

STOTHERS, R ^{[1
]}

机构：

[1] NASA,GODDARD SPACE FLIGHT CTR,INST SPACE STUDIES,2880 BROADWAY,NEW YORK,NY 10025

来源：

ASTROPHYSICAL JOURNAL | 1974年 / 192卷 / 01期

关键词：

D O I：

10.1086/153044

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：145 / 148

页数：4

共 16 条

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[4]

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[5]

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Pekeris, CL .

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[7] ON THE RADIAL PULSATION OF GASEOUS STARS [J].

LEDOUX, P .

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[8]

LEDOUX P, 1958, HDB PHYSIK, V51

[9] STRUCTURE AND EVOLUTION OF RAPIDLY ROTATING B-TYPE STARS [J].

SACKMANN, IJ ;

ANAND, SPS .

ASTROPHYSICAL JOURNAL, 1970, 162 (01) :105-&

[10] ON THE MAXIMUM MASS OF STABLE STARS [J].

SCHWARZSCHILD, M ;

HARM, R .

ASTROPHYSICAL JOURNAL, 1959, 129 (03) :637-646

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