a Temperature gradient in close binary systems

被引：0

作者：

Rovithis-Livaniou, H. ^{[1
]}

Kalimeris, A. ^{[2
]}

机构：

[1] Univ Athens, Fac Phys, Dept Astrophys Astron & Mech, Athens, Greece

[2] Inst Lonian Islands, Technol & Educ, Zakynthos, Greece

来源：

FIFTY YEARS OF ROMANIAN ASTROPHYSICS | 2007年 / 895卷

关键词：

stars; binaties-stars; surface gravity-stars; temperature gradient;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The influence of the gravity darkening effect in the formation of a non iso-thermal photosphere on close binary stars is presented. Furthermore, a theoretical model that describes thermal differences on the stars' surfaces, based on the temperature gradient equations, has been constructed. Application on TY Pup has been made and presented.

引用

页码：247 / +

页数：3

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