CONSEQUENCES OF MASS-TRANSFER IN CLOSE BINARY-SYSTEMS

被引:74
作者
THOMAS, HC [1 ]
机构
[1] MAX PLANCK INST PHYS & ASTROPHYS,D-8000 MUNICH 40,FED REP GER
关键词
D O I
10.1146/annurev.aa.15.090177.001015
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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页码:127 / 151
页数:25
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共 156 条
[1]   MULTIPLICITY AMONG SOLAR-TYPE STARS [J].
ABT, HA ;
LEVY, SG .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1976, 30 (03) :273-306
[2]   ORBITAL EVOLUTION OF A SINGLY CONDENSED, CLOSE BINARY, BY MASS-LOSS FROM PRIMARY AND BY ACCRETION DRAG ON CONDENSED MEMBER [J].
ALEXANDER, ME ;
CHAU, WY ;
HENRIKSEN, RN .
ASTROPHYSICAL JOURNAL, 1976, 204 (03) :879-888
[3]   POSSIBLE MECHANISM FOR MASS-TRANSFER IN X-RAY BINARY-SYSTEMS WITH OB SUPERGIANT COMPANIONS [J].
ALME, ML ;
WILSON, JR .
ASTROPHYSICAL JOURNAL, 1976, 210 (01) :233-238
[4]  
AMNUEL PR, 1976, ASTRON ASTROPHYS, V46, P163
[5]  
[Anonymous], 1964, B ASTRON I CZECH
[6]  
[Anonymous], 1976, IAU S 73 STRUCT EV
[7]  
[Anonymous], ACA
[8]  
[Anonymous], MULTIPLE PERIODIC VA
[9]  
[Anonymous], 1956, ANN DASTROPHYSIQUE
[10]  
Arnett W. D., 1973, EXPLOSIVE NUCLEOSYNT, P236