THE COMPUTATION OF MOLECULAR ABUNDANCES AND OPACITIES IN THE ATMOSPHERES OF LATE-TYPE STARS

被引：0
|
作者：
SHARP, CM
机构：
来源：
IAU SYMPOSIA | 1987年 / 120期
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
引用
收藏
页码：407 / 408
页数：2
相关论文
共 50 条
  • [31] TECHNETIUM IN LATE-TYPE STARS
    BAJCAR, R
    JOURNAL OF THE ROYAL ASTRONOMICAL SOCIETY OF CANADA, 1969, 63 (04) : 211 - &
  • [32] HA IN LATE-TYPE STARS
    PRICE, MJ
    OBSERVATORY, 1967, 87 (956): : 18 - &
  • [33] SUBLUMINOUS LATE-TYPE STARS
    EGGEN, OJ
    ASTROPHYSICAL JOURNAL, 1968, 153 (1P1): : 195 - &
  • [34] Observations of late-type stars
    Cohen, M
    DIFFUSE INFRARED RADIATION AND THE IRTS, 1997, 124 : 61 - 66
  • [35] Isochrones for late-type stars
    Demarque, Pierre
    AGES OF STARS, 2009, (258): : 383 - 394
  • [36] Constraints on the use of Be I lines for deriving beryllium abundances in late-type dwarf stars
    Lopez, RJG
    ASTRONOMY & ASTROPHYSICS, 1996, 313 (03) : 909 - 912
  • [37] Chemical abundances of late-type pre-main sequence stars in the σ Orionis cluster
    González Hernández, J.I.
    Caballero, J.A.
    Rebolo, R.
    Béjar, V.J.S.
    Barrado Y Navascués, D.
    Martín, E.L.
    Zapatero Osorio, M.R.
    Astronomy and Astrophysics, 2008, 490 (03): : 1135 - 1142
  • [38] Chemical abundances of late-type pre-main sequence stars in the σ Orionis cluster
    Gonzalez Hernandez, J. I.
    Caballero, J. A.
    Rebolo, R.
    Bejar, V. J. S.
    Barrado y Navascues, D.
    Martin, E. L.
    Zapatero Osorio, M. R.
    ASTRONOMY & ASTROPHYSICS, 2008, 490 (03) : 1135 - 1142
  • [39] A non-LTE analysis of Mg I lines in the atmospheres of late-type stars
    Mashonkina, LI
    Shimanskaya, NN
    Sakhibullin, NA
    ASTRONOMICHESKII ZHURNAL, 1996, 73 (02): : 212 - 220
  • [40] CONSEQUENCES OF GRAINS IN ATMOSPHERES OF LATE-TYPE STARS .2. THERMODYNAMICS OF GRAINS IN A CHROMOSPHERE
    JENNINGS, MC
    ASTROPHYSICAL JOURNAL, 1973, 185 (01): : 197 - 207
12345