H-EMISSION AND K-EMISSION IN LATE-TYPE STARS - DEPENDENCE OF LINE WIDTH ON LUMINOSITY AND RELATED TOPICS

被引:420
|
作者
WILSON, OC
BAPPU, MKV
机构
来源
ASTROPHYSICAL JOURNAL | 1957年 / 125卷 / 03期
关键词
D O I
10.1086/146339
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:661 / &
相关论文
共 50 条
  • [41] Hα emission from late type Be stars
    Apparao, KMV
    Tarafdar, SP
    JOURNAL OF ASTROPHYSICS AND ASTRONOMY, 1997, 18 (2-3) : 145 - 150
  • [42] S-I EMISSION IN EUV SPECTRA OF LATE-TYPE STARS
    BROWN, A
    JORDAN, C
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1980, 191 (03) : P37 - P41
  • [43] Peculiarities of the plasma mechanism of radio emission from late-type stars
    V. V. Zaitsev
    E. G. Kupriyanova
    A. V. Stepanov
    Astronomy Letters, 2000, 26 : 736 - 742
  • [44] MICROWAVE OH MASER EMISSION IN THE CIRCUMSTELLAR ENVELOPES OF LATE-TYPE STARS
    BOWERS, PF
    JOHNSTON, KJ
    SPENCER, JH
    NATURE, 1981, 291 (5814) : 382 - 385
  • [45] Highly polarized SiO ν=0 emission from late-type stars
    Shinnaga, H
    Tsuboi, M
    Kasuga, T
    COSMIC MASERS: FROM PROTOSTARS TO BLACKHOLES, 2002, (206): : 278 - 281
  • [46] THE CIRCUMSTELLAR H2O MASER EMISSION ASSOCIATED WITH 4 LATE-TYPE STARS
    JOHNSTON, KJ
    SPENCER, JH
    BOWERS, PF
    ASTROPHYSICAL JOURNAL, 1985, 290 (02): : 660 - 670
  • [47] OPTICAL AND RADIO ASTROMETRY OF 4 LATE-TYPE STARS WITH MASER EMISSION
    DEVEGT, C
    KLEINE, T
    JOHNSTON, KJ
    BOWERS, PF
    SPENCER, JH
    ASTRONOMY & ASTROPHYSICS, 1987, 179 (1-2) : 322 - 328
  • [48] COPERNICUS SURVEY OF MG-II EMISSION IN LATE-TYPE STARS
    WEILER, EJ
    OEGERLE, WR
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1979, 39 (04): : 537 - 547
  • [49] Peculiarities of the plasma mechanism of radio emission from late-type stars
    Zaitsev, VV
    Kupriyanova, EG
    Stepanov, AV
    ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS, 2000, 26 (11): : 736 - 742
  • [50] OBSERVATIONS OF 86 GHZ SIO MASER EMISSION IN LATE-TYPE STARS
    LEBERTRE, T
    NYMAN, LA
    ASTRONOMY & ASTROPHYSICS, 1990, 233 (02) : 477 - 485