Non-spherical radiation-driven wind models

被引：0

作者：

Puls, J ^{[1
]}

Petrenz, P ^{[1
]}

Owocki, SP ^{[1
]}

机构：

[1] Universitatssternwarte, D-81679 Munich, Germany

来源：

VARIABLE AND NON-SPHERICAL STELLAR WINDS IN LUMINOUS HOT STARS | 1999年 / 523卷

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：

The present state of modelling radiatively driven stellar winds from rapidly rotating stars is reviewed. Various processes affecting the actual, still controversial wind structure are highlighted, in particular non-radial line-forces and gravity darkening, and useful scaling relations are provided. The importance of accounting for consistent NLTE line-forces depending both on the actual density structure and radiation field (as function of latitude and radius) is stressed, and some independent test calculations confirming earlier numerical results are reported.

引用

页码：131 / 139

页数：9

共 18 条

[1] EQUATORIAL DISK FORMATION AROUND ROTATING STARS DUE TO RAM PRESSURE CONFINEMENT BY THE STELLAR WIND [J].