THE POST-RLOF STRUCTURE OF THE SECONDARY COMPONENTS IN CLOSE BINARY-SYSTEMS, WITH AN APPLICATION TO MASSES OF WOLF-RAYET STARS

被引：35

作者：

HELLINGS, P

机构：

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1984年 / 104卷 / 01期

关键词：

D O I：

10.1007/BF00653994

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

收藏

页码：83 / 109

页数：27

相关论文

共 42 条

[1] BARBARO G, 1969, MASS LOSS STARS, P217
[2] MASS-LOSS RATES FOR 21 WOLF-RAYET STARS
BARLOW, MJ
SMITH, LJ
WILLIS, AJ
[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1981, 196 (01) : 101 - 110
[3] AN ORBIT FOR THE WC7 WOLF-RAYET BINARY HD-97152 - COMPARISON WITH THE SINGLE-LINE WC7 STAR HD-156385
DAVIS, AB
MOFFAT, AFJ
NIEMELA, VS
[J]. ASTROPHYSICAL JOURNAL, 1981, 244 (02) : 528 - 540
[4] DELOORE C, 1981, IAU C, V59, P408
[5] DELOORE C, 1976, ASTROPHYS SPACE SCI, V35, P241
[6] ON THE EVOLUTIONARY TIME SCALE OF THE ACCRETING COMPONENT IN MASSIVE CLOSE BINARIES
DOOM, C
DEGREVE, JP
[J]. ASTROPHYSICS AND SPACE SCIENCE, 1981, 80 (02) : 369 - 395
[7] FRAQUELLI DA, 1983, UNPUB
[8] GANESH VS, 1967, KODAIKANAL OBSERV A, P184
[9] GAPOSCHKIN S, 1949, PEREM ZVEZDY, V7, P36
[10] PHENOMENOLOGICAL STUDY OF MASSIVE ACCRETION STARS
HELLINGS, P
[J]. ASTROPHYSICS AND SPACE SCIENCE, 1983, 96 (01) : 37 - 54

← 1 2 3 4 5 →