Ambient magnetic fields and dynamos: Pre-main sequence stars and elsewhere

被引:0
|
作者
机构
[1] Moss, D.
来源
Moss, D. (moss@ma.man.ac.uk) | 1600年 / EDP Sciences卷 / 414期
关键词
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
  • [31] Luminous pre-main sequence stars in the LMC?
    Lamers, HJGLM
    Beaulieu, JP
    de Wit, WJ
    ASTRONOMY & ASTROPHYSICS, 1999, 341 (03): : 827 - 841
  • [32] Pre-main sequence stars in LH 91
    Carini, R.
    Biazzo, K.
    De Marchi, G.
    Panagia, N.
    Beccari, G.
    Brocato, E.
    ASTRONOMY & ASTROPHYSICS, 2022, 663
  • [33] Pre-Main Sequence Stars Seen by ISO
    Dario Lorenzetti
    Space Science Reviews, 2005, 119 : 181 - 199
  • [34] The survival of fossil magnetic fields during pre-main sequence evolution
    Moss, D
    ASTRONOMY & ASTROPHYSICS, 2003, 403 (02) : 693 - 697
  • [35] Chemical peculiarities in magnetic and non-magnetic pre-main sequence A and B stars
    Folsom, C. P.
    Bagnulo, S.
    Wade, G. A.
    Landstreet, J. D.
    Alecian, E.
    MAGNETIC FIELDS THROUGHOUT STELLAR EVOLUTION, 2014, (302): : 87 - 90
  • [37] MOST results for some pre-main sequence stars
    Siwak, M.
    Rucinski, S. M.
    Matthews, J. M.
    Cameron, C.
    Guenther, D. B.
    Kuschnig, R.
    Weiss, W. W.
    Moffat, A. F. J.
    Rowe, J. F.
    Sasselov, D.
    Drozdz, M.
    Ogloza, W.
    SECOND BRITE-CONSTELLATION SCIENCE CONFERENCE - SMALL SATELLITES - BIG SCIENCE, 2017, 5 : 214 - 216
  • [38] Convection in the atmospheres and envelopes of Pre-Main Sequence stars
    Montalbán, J
    D'Antona, F
    Kupka, F
    Heiter, U
    ASTRONOMY & ASTROPHYSICS, 2004, 416 (03) : 1081 - 1096
  • [40] Loss of angular momentum of magnetic Ap stars in the pre-main sequence phase
    Stepien, K
    ASTRONOMY & ASTROPHYSICS, 2000, 353 (01): : 227 - 238