Physics of radiatively driven winds by High Angular Resolution Observations (HARO)

被引：0

作者：

Stee, P ^{[1
]}

Bonneau, D ^{[1
]}

Mourard, D ^{[1
]}

Vakili, F ^{[1
]}

机构：

[1] Observ Cote Azur, CNRS, UMR 6528, Equip G12T,Dept Fresnel, F-06460 St Vallier Thiey, France

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：

Numerous models have been developed during the last two decades which try to fit a small number of "classical" observables as closely as possible (i.e Her line profile and continuum energy distribution or polarization data). Nevertheless, little has been done to include High Angular Resolution Observations (HARO) in simulations in spite of the fact that such data can strongly constrain radiative mind models. rn the following, we shall review recent results coming from HARO of active B stars and we shall focus on our radiative mind model for active hot stars which integrates these measurements.

引用

页码：115 / 118

页数：4

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