EVOLUTION OF MASSIVE STARS WITH LOW METAL ABUNDANCE HOLDING FOR THE MAGELLANIC CLOUDS

被引：0
|
作者：
HELLINGS, P
VANBEVEREN, D
机构：
来源：
ASTRONOMY & ASTROPHYSICS | 1981年 / 95卷 / 01期
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
引用
收藏
页码：14 / 17
页数：4
相关论文
共 50 条
  • [21] MASSIVE CLOSE BINARY EVOLUTION IN THE GALAXY AND IN THE MAGELLANIC CLOUDS
    DELOORE, C
    VANBEVEREN, D
    ASTRONOMY & ASTROPHYSICS, 1994, 292 (02) : 463 - 470
  • [22] THE CLOSE BINARY PROPERTIES OF MASSIVE STARS IN THE MILKY WAY AND LOW-METALLICITY MAGELLANIC CLOUDS
    Moe, Maxwell
    Di Stefano, Rosanne
    ASTROPHYSICAL JOURNAL, 2013, 778 (02):
  • [23] THEORETICAL EVOLUTION OF MASSIVE STARS WITH LOW METAL CONTENT
    ALCOCK, C
    PACZYNSKI, B
    BULLETIN OF THE AMERICAN PHYSICAL SOCIETY, 1975, 20 (01): : 17 - 17
  • [24] THE MAGELLANIC CLOUDS .16. INFRARED STARS AND STELLAR EVOLUTION
    SHAPLEY, H
    PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 1955, 41 (11) : 824 - 828
  • [25] THE BRIGHTEST STARS IN THE MAGELLANIC CLOUDS
    FEAST, MW
    THACKERAY, AD
    WESSELINK, AJ
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1960, 121 (04) : 337 - &
  • [26] A study of Be stars in the Magellanic Clouds
    Iqbal, S.
    Keller, S. C.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2013, 435 (04) : 3103 - 3110
  • [27] CMFGEN grids of atmosphere models for massive stars: OB-Type stars at the Magellanic Clouds
    Marcolino, W.
    Bouret, J.-C.
    Martins, F.
    Hillier, D.J.
    Astronomy and Astrophysics, 2024, 690
  • [28] EXTREME BE STARS IN THE MAGELLANIC CLOUDS
    GARMANY, CD
    HUMPHREYS, RM
    ASTRONOMICAL JOURNAL, 1985, 90 (10): : 2009 - &
  • [29] CMFGEN grids of atmosphere models for massive stars: OB-type stars at the Magellanic Clouds
    Marcolino, W.
    Bouret, J. -C
    Martins, F.
    Hillier, D. J.
    ASTRONOMY & ASTROPHYSICS, 2024, 690
  • [30] Carbon stars in the Magellanic Clouds
    Azzopardi, M
    NEW VIEWS OF THE MAGELLANIC CLOUDS, 1999, (190): : 324 - 327
12345