EVOLUTION OF LOW-MASS CLOSE BINARY-SYSTEMS .4. 0.80 M. AND 0.40 M. - CATASTROPHIC MASS-LOSS

被引:37
作者
WEBBINK, RF
机构
[1] UNIV ILLINOIS,DEPT ASTRON,URBANA,IL 61801
[2] UNIV CAMBRIDGE,INST ASTRON,CAMBRIDGE,ENGLAND
关键词
D O I
10.1086/154998
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:881 / 889
页数:9
相关论文
共 18 条
[1]  
[Anonymous], 1967, MCOMP
[3]   DYNAMICAL INSTABILITIES AND MASS EXCHANGE IN BINARY-SYSTEMS [J].
BATH, GT .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1975, 171 (02) :311-328
[5]   STELLAR ACCRETION AND X-RAY EMISSION [J].
CAMERON, AGW ;
MOCK, M .
NATURE, 1967, 215 (5100) :464-&
[6]   LOCATION OF HOT SPOT IN CATACLYSMIC VARIABLE-STARS AS DETERMINED FROM PARTICLE TRAJECTORIES [J].
FLANNERY, BP .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1975, 170 (02) :325-331
[7]  
Jedrzejec E., 1969, THESIS WARSAW U
[8]  
KRIZ S, 1968, B ASTRON I CZECH, V19, P248
[9]  
Landau L. D., 1959, FLUID MECHANICS, p[xii, 536]
[10]  
NARIAI K, 1967, PUBL ASTRON SOC JPN, V19, P564