THE SIZE OF CONVECTIVE CORES IN ROTATING STELLAR MODELS

被引:5
作者
SREENIVASAN, SR
WILSON, WJF
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D O I
10.1086/167552
中图分类号
P1 [天文学];
学科分类号
0704 ;
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页码:939 / 947
页数:9
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[1]  
ANAND SPS, 1970, APJ, V162, P105
[2]   RAPIDLY ROTATING STARS .7. EFFECTS OF ANGULAR MOMENTUM ON UPPER-MAIN-SEQUENCE MODELS [J].
BODENHEIMER, P .
ASTROPHYSICAL JOURNAL, 1971, 167 (01) :153-+
[3]  
Cox J. P., 1968, PRINCIPLES STELLAR S, V1
[4]   EVOLUTION OF ROTATING STARS .2. CALCULATIONS WITH TIME-DEPENDENT REDISTRIBUTION OF ANGULAR-MOMENTUM FOR 7 AND 10 MBY STARS [J].
ENDAL, AS ;
SOFIA, S .
ASTROPHYSICAL JOURNAL, 1978, 220 (01) :279-290
[5]   EVOLUTION OF ROTATING STARS .1. METHOD AND EXPLORATORY CALCULATIONS FOR A 7M. STAR [J].
ENDAL, AS ;
SOFIA, S .
ASTROPHYSICAL JOURNAL, 1976, 210 (01) :184-198
[6]  
Kippenhahn R., 1970, STELLAR ROTATION
[7]   ON THE SIZE OF CONVECTIVE CORES IN ROTATING, UPPER-MAIN-SEQUENCE STARS [J].
MACGREGOR, KB ;
GILLILAND, RL .
ASTROPHYSICAL JOURNAL, 1986, 310 (01) :273-276
[8]  
NARASIMHA D, 1988, UNPUB
[9]  
NARASIMHA D, 1987, STELLAR PULSATION ME, P106
[10]   Proposal of a New Method of Solution of the Unsteady Non-linear Eddington-Vogt-Sweet Circulation [J].
Sakurai, Takeo .
GEOPHYSICAL AND ASTROPHYSICAL FLUID DYNAMICS, 1986, 36 (3-4) :257-301