STABILITY OF MASSIVE STARS AND THE HUMPHREYS-DAVIDSON LIMIT

被引:77
作者
GLATZEL, W
KIRIAKIDIS, M
机构
关键词
INSTABILITIES; STARS-OSCILLATIONS; STARS-SUPERGIANTS; STARS-VARIABLES; OTHER;
D O I
10.1093/mnras/263.2.375
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using standard physics and opacities, the stability of massive stars is re-examined. Violent mode-coupling instabilities are identified which could account for the LBV phenomenon. The stability boundary seems to be related to the Humphreys-Davidson limit.
引用
收藏
页码:375 / 384
页数:10
相关论文
共 42 条
[1]  
APPENZELLER I, 1970, ASTRON ASTROPHYS, V5, P355
[2]  
APPENZELLER I, 1986, P IAU S, V116, P139
[3]   PULSATIONS OF MODELS OF DELTA CEPHEI STARS .2. [J].
BAKER, N ;
KIPPENHA.R .
ASTROPHYSICAL JOURNAL, 1965, 142 (03) :868-&
[4]  
Baker N., 1962, ZAP, V54, P114
[5]   AN OPACITY MECHANISM FOR THE PULSATIONS OF OB STARS [J].
COX, AN ;
MORGAN, SM ;
ROGERS, FJ ;
IGLESIAS, CA .
ASTROPHYSICAL JOURNAL, 1992, 393 (01) :272-277
[6]  
Cox J. P., 1980, THEORY STELLAR PULSA, DOI [DOI 10.1515/9781400885855, 10.1515/9781400885855]
[7]   THE RELATION BETWEEN APPARENT TEMPERATURE AND MASS-LOSS RATE IN HYPERGIANT ERUPTIONS [J].
DAVIDSON, K .
ASTROPHYSICAL JOURNAL, 1987, 317 (02) :760-764
[8]  
de Jager C., 1980, THE BRIGHTEST STARS
[9]  
DEJAGER C, 1984, ASTRON ASTROPHYS, V138, P246
[10]  
GAUTSCHY A, 1990, MON NOT R ASTRON SOC, V245, P154