Balmer line profiles as stellar atmosphere structure indicators

被引:0
作者
van't Veer-Menneret, C [1 ]
Katz, D [1 ]
机构
[1] Observ Paris, DASGAL, F-75014 Paris, France
来源
THEORY AND TESTS OF CONVECTION IN STELLAR STRUCTURE: FIRST GRANADA WORKSHOP | 1999年 / 173卷
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P1 [天文学];
学科分类号
0704 ;
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页码:209 / 212
页数:4
相关论文
共 14 条
[1]  
AXER M, 1994, ASTRON ASTROPHYS, V291, P895
[2]  
Bernkopf J, 1998, ASTRON ASTROPHYS, V332, P127
[3]   STELLAR TURBULENT CONVECTION - A NEW MODEL AND APPLICATIONS [J].
CANUTO, VM ;
MAZZITELLI, I .
ASTROPHYSICAL JOURNAL, 1991, 370 (01) :295-311
[4]  
Castelli F, 1997, ASTRON ASTROPHYS, V318, P841
[5]  
FUHRMANN K, 1994, ASTRON ASTROPHYS, V285, P585
[6]  
Fuhrmann K, 1997, ASTRON ASTROPHYS, V323, P909
[7]  
FUHRMANN K, 1993, ASTRON ASTROPHYS, V271, P451
[8]  
GIRARD T, 1996, BAAS, V28, P919
[9]  
KURUCZ RL, CD ROM, V13, P14
[10]  
Lebreton Y, 1997, ESA SP PUBL, V402, P379