LIMB-DARKENING FOR COOL STARS - STANDARD AND IRRADIATED MODELS

被引:1
作者
CLARET, A
GIMENEZ, A
机构
[1] Instituto de Astrofisica de Andalucía, Granada
关键词
D O I
10.1007/BF00640718
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Limb-darkening coefficients for a grid of LTE, non-grey atmosphere models has been calculated by means of Upsalla Model Atmosphere (UMA) code using a least-squares fitting. Both linear and quadratic laws were adopted in the standard models and in those with irradiation from a companion, star as well, more realistic for the case of close binaries. © 1990 Kluwer Academic Publishers.
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页码:223 / 225
页数:3
相关论文
共 8 条
[1]  
Allen C.W., 1973, ASTROPHYSICAL QUANTI
[2]  
DIAZCORDOBES J, 1990, UNPUB
[3]  
GIMENEZ A, 1988, IAU C, V107, P343
[4]  
GUSTAFSSON B, 1975, ASTRON ASTROPHYS, V42, P407
[6]  
MANDUCA A, 1977, ASTRON ASTROPHYS, V61, P809
[7]  
VAZ LPR, 1985, ASTRON ASTROPHYS, V147, P281
[8]  
Wade R. A., 1985, Astronomy & Astrophysics Supplement Series, V60, P471