THE LINE-PROFILE VARIATIONS OF SPICA

被引：12
|
作者：
WALKER, GAH
MOYLES, K
YANG, S
FAHLMAN, GG
机构：
来源：
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 1982年 / 94卷 / 557期
关键词：
D O I：
10.1086/130953
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
引用
收藏
页码：143 / 148
页数：6
相关论文
共 50 条
  • [1] THE LINE-PROFILE VARIATIONS OF SPICA
    WALKER, GAH
    MOYLES, K
    YANG, S
    FAHLMAN, GG
    [J]. JOURNAL OF THE ROYAL ASTRONOMICAL SOCIETY OF CANADA, 1981, 75 (05) : 254 - 254
  • [2] LINE-PROFILE VARIATIONS IN BE STARS
    GIES, DR
    [J]. PULSATION, ROTATION AND MASS LOSS IN EARLY-TYPE STARS, 1994, (162): : 89 - 99
  • [3] LINE-PROFILE VARIATIONS IN BE STARS
    APPARAO, KMV
    TARAFDAR, SP
    [J]. ASTROPHYSICS AND SPACE SCIENCE, 1989, 153 (01) : 61 - 66
  • [4] LINE-PROFILE VARIABILITY FROM TIDAL FLOWS IN ALPHA VIRGINIS (SPICA)
    Harrington, David
    Koenigsberger, Gloria
    Moreno, Edmundo
    Kuhn, Jeffrey
    [J]. ASTROPHYSICAL JOURNAL, 2009, 704 (01): : 813 - 830
  • [5] Mode detection from line-profile variations
    Mantegazza, L
    [J]. DELTA SCUTI AND RELATED STARS: REFERENCE HANDBOOK AND PROCEEDINGS OF THE 6TH VIENNA WORKSHOP IN ASTROPHYSICS, 2000, 210 : 138 - 169
  • [6] Mode identification from line-profile variations
    Aerts, C
    Eyer, L
    [J]. DELTA SCUTI AND RELATED STARS: REFERENCE HANDBOOK AND PROCEEDINGS OF THE 6TH VIENNA WORKSHOP IN ASTROPHYSICS, 2000, 210 : 113 - 137
  • [7] LINE-PROFILE VARIATIONS OF ROTATING, PULSATING STARS
    AERTS, C
    WAELKENS, C
    [J]. ASTRONOMY & ASTROPHYSICS, 1993, 273 (01) : 135 - 146
  • [8] The line-profile variations of theta(2) Tauri
    Kennelly, EJ
    Walker, GAH
    [J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1996, 108 (722) : 327 - 331
  • [9] Spatial wavelet analysis of line-profile variations
    Townsend, RHD
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1999, 310 (03) : 851 - 862
  • [10] TAU PEGASI - A FOURIER REPRESENTATION OF LINE-PROFILE VARIATIONS
    KENNELLY, EJ
    WALKER, GAH
    MERRYFIELD, WJ
    [J]. ASTROPHYSICAL JOURNAL, 1992, 400 (02): : L71 - L74
12345