THE EVOLUTION OF EARLY MAIN-SEQUENCE STARS

被引：67

|

作者：

KUSHWAHA, RS

机构：

来源：

ASTROPHYSICAL JOURNAL | 1957年 / 125卷 / 01期

关键词：

D O I：

10.1086/146298

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

收藏

页码：242 / 259

页数：18

相关论文

共 50 条

[31] Diffusion and Mixing in Main-Sequence Stars
Sylvie Vauclair
Astrophysics and Space Science, 2003, 284 : 205 - 215
[32] THE STABILITY OF MASSIVE MAIN-SEQUENCE STARS
GLATZEL, W
KIRIAKIDIS, M
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1993, 262 (01) : 85 - 92
[33] Evolution of the magnetic fields of main-sequence CP-stars. II
Glagolevskij, Yu. V.
ASTROPHYSICS, 2013, 56 (03) : 407 - 420
[34] ON THE INITIAL DISTRIBUTION AND EVOLUTION OF ANGULAR-MOMENTUM FOR MAIN-SEQUENCE STARS
CARRASCO, L
FRANCO, J
ROTH, M
ASTRONOMY & ASTROPHYSICS, 1980, 86 (1-2) : 217 - 220
[35] Evolution of the Magnetic Fields of Main-Sequence CP-Stars. IV
Glagolevskij, Yu V.
ASTROPHYSICS, 2014, 57 (03) : 315 - 329
[36] Evolution of the Magnetic Fields of Main-Sequence CP-Stars. IV
Yu. V. Glagolevskij
Astrophysics, 2014, 57 : 315 - 329
[37] Evolution of the magnetic fields of main-sequence CP-stars. II
Yu. V. Glagolevskij
Astrophysics, 2013, 56 : 407 - 420
[38] An analysis of the incidence of the Vega phenomenon among main-sequence and post main-sequence stars
Plets, H
Vynckier, C
ASTRONOMY & ASTROPHYSICS, 1999, 343 (02): : 496 - 506
[39] Evolution of the Magnetic Fields of Main-Sequence CP-Stars. V
Glagolevskij, Yu. V.
ASTROPHYSICS, 2015, 58 (01) : 29 - 45
[40] EVOLUTION FROM MAIN-SEQUENCE TO HELIUM FLASH FOR POPULATION II STARS
DEMARQUE, P
MENGEL, JG
ASTRONOMY & ASTROPHYSICS, 1973, 22 (01) : 121 - 128

← 1 2 3 4 5 →