Massive star evolution in close binaries: Conditions for homogeneous chemical evolution

被引:0
|
作者
Song, H.F. [1 ,3 ]
Meynet, G. [2 ]
Maeder, A. [2 ]
Ekström, S. [2 ]
Eggenberger, P. [2 ]
机构
[1] College of Science, Guizhou University, Guiyang, Guizhou Province,550025, China
[2] Geneva Observatory, Geneva University, Sauverny,1290, Switzerland
[3] Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming,650011, China
来源
Astronomy and Astrophysics | 2016年 / 585卷
关键词
30;
D O I
暂无
中图分类号
学科分类号
摘要
引用
收藏
相关论文
共 50 条
  • [41] Evolution of Very Close Binaries of Low Mass
    Eggleton, Peter P.
    BINARIES - KEY TO COMPREHENSION OF THE UNIVERSE, 2010, 435 : 151 - 160
  • [42] FK-COMAE AND THE EVOLUTION OF CLOSE BINARIES
    HUENEMOERDER, DP
    RAMSEY, LW
    BUZASI, DL
    NATIONS, HL
    IAU SYMPOSIA, 1992, (151): : 403 - 406
  • [43] Evolution of Cool Close Binaries - Approach to Contact
    Stepien, K.
    ACTA ASTRONOMICA, 2011, 61 (02): : 139 - 159
  • [44] THE EVOLUTION OF MODERATELY CLOSE AND MODERATELY WIDE BINARIES
    EGGLETON, PP
    TOUT, CA
    SPACE SCIENCE REVIEWS, 1989, 50 (1-2) : 165 - 177
  • [45] The chemical evolution of the secondary stars in close binaries, arising from common-envelope evolution and nova outbursts
    Marks, PB
    Sarna, MJ
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1998, 301 (03) : 699 - 720
  • [46] Very massive close binaries and the puzzling temporal evolution of 14N in the Solar Neighbourhood
    Vanbeveren, D.
    De Donder, E.
    NEW ASTRONOMY, 2006, 12 (02) : 95 - 103
  • [48] THE EVOLUTION OF MASSIVE CLOSE BINARY STARS
    TUTUKOV, AV
    MASEVICH, AG
    USPEKHI FIZICHESKIKH NAUK, 1980, 132 (02): : 390 - 391
  • [49] Chemical evolution in the early phases of massive star formation. I
    Gerner, T.
    Beuther, H.
    Semenov, D.
    Linz, H.
    Vasyunina, T.
    Bihr, S.
    Shirley, Y. L.
    Henning, Th.
    ASTRONOMY & ASTROPHYSICS, 2014, 563
  • [50] The influence of binaries on galactic chemical evolution
    De Donder, E
    Vanbeveren, D
    NEW ASTRONOMY REVIEWS, 2004, 48 (10) : 861 - 975