ON SECOND HELIUM IONIZATION AS A CAUSE OF PULSATIONAL INSTABILITY IN STARS

被引：56
|
作者：
COX, JP
机构：
来源：
ASTROPHYSICAL JOURNAL | 1963年 / 138卷 / 02期
关键词：
D O I：
10.1086/147661
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
引用
收藏
页码：487 / &
相关论文
共 50 条
  • [41] Nonlinear pulsational characteristics of HADS stars
    Antonello, E
    DELTA SCUTI AND RELATED STARS: REFERENCE HANDBOOK AND PROCEEDINGS OF THE 6TH VIENNA WORKSHOP IN ASTROPHYSICS, 2000, 210 : 381 - 390
  • [42] Pulsational Pair-instability Supernovae
    Woosley, S. E.
    ASTROPHYSICAL JOURNAL, 2017, 836 (02):
  • [43] Turbulent convection and pulsational stability of variable stars -: IV.: The red edge of the δ Scuti instability strip
    Xiong, DR
    Deng, L
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2001, 324 (01) : 243 - 248
  • [44] Pulsational instability of high-luminosity H-rich pre-white dwarf stars
    Calcaferro, Leila M.
    Corsico, Alejandro H.
    Camisassa, Maria E.
    Althaus, Leandro G.
    Shibahashi, Hiromoto
    WIDE-FIELD VARIABILITY SURVEYS: A 21ST CENTURY PERSPECTIVE, 2017, 152
  • [45] TURBULENT CONVECTION AND PULSATIONAL STABILITY OF VARIABLE STARS
    熊大闰
    ScienceinChina,SerA., 1980, Ser.A.1980 (09) : 1139 - 1149
  • [46] Pulsational instability domain of δ Scuti variables
    Pamyatnykh, AA
    DELTA SCUTI AND RELATED STARS: REFERENCE HANDBOOK AND PROCEEDINGS OF THE 6TH VIENNA WORKSHOP IN ASTROPHYSICS, 2000, 210 : 215 - 246
  • [47] Pulsational properties of cluster RR Lyrae stars
    Petroni, S
    Bono, G
    Castellani, V
    NEW HORIZONS IN GLOBULAR CLUSTER ASTRONOMY, 2003, 296 : 397 - 399
  • [48] TURBULENT CONVECTION AND PULSATIONAL STABILITY OF VARIABLE STARS
    熊大闰
    Science China Mathematics, 1980, (09) : 1139 - 1149
  • [49] PULSATIONAL PROPERTIES OF POST-AGB STARS
    ZALEWSKI, J
    ACTA ASTRONOMICA, 1993, 43 (04): : 431 - 440
  • [50] A pulsational study of crystallized white dwarf stars
    Montgomery, MH
    Winget, DE
    HALF CENTURY OF STELLAR PULSATION INTERPRETATIONS: A TRIBUTE TO ARTHUR N. COX, 1998, 135 : 449 - 450
12345