BETA PERSEI - RADIO STAR AND PROBABLE X-RAY STAR

被引:23
作者
HJELLMING, RM
机构
来源
NATURE-PHYSICAL SCIENCE | 1972年 / 238卷 / 82期
关键词
D O I
10.1038/physci238052a0
中图分类号
Q6 [生物物理学];
学科分类号
071011 ;
摘要
引用
收藏
页码:52 / +
页数:1
相关论文
共 19 条
  • [1] HA EMISSION IN ALGOL
    ANDREWS, PJ
    [J]. ASTROPHYSICAL JOURNAL, 1967, 147 (03) : 1183 - &
  • [2] BOLTON CT, 1972, 2388 INT ASTR UN CIR
  • [3] Conner J. P., 1969, Astrophysical Journal, V157, pl157, DOI 10.1086/180409
  • [4] OBSERVATIONS OF DEVELOPMENT AND DISAPPEARANCE OF X-RAY SOURCE CENTAURUS-XR-4
    EVANS, WD
    BELIAN, RD
    CONNER, JP
    [J]. ASTROPHYSICAL JOURNAL, 1970, 159 (1P2) : L57 - &
  • [5] FRIEBOES.H, 1970, ASTRON ASTROPHYS, V4, P78
  • [6] GLUSHNEVA IN, 1968, SOV ASTRON, V11, P828
  • [7] HERCZEG T, 1968, NONPERIODIC PHENOMEN
  • [8] RADIO VARIATIONS OF BETA-PERSEI AND BETA-LYRAE
    HJELLMING, RM
    WEBSTER, E
    WADE, CM
    [J]. NATURE-PHYSICAL SCIENCE, 1972, 236 (64): : 43 - +
  • [9] HUGHES, 1972, NATURE PHYSICAL SCIE, V236, P42
  • [10] ENERGY SPECTRUM OF A NOVA-LIKE X-RAY SOURCE
    KITAMURA, T
    NAKAGAWA, M
    TAKAGISHI, K
    MATSUOKA, M
    MIYAMOTO, S
    ODA, M
    OGAWARA, Y
    [J]. NATURE, 1971, 229 (5279) : 31 - +