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A clump model for Wolf-Rayet star atmospheres

Published online by Cambridge University Press:  07 August 2017

A. F. Kholtygin
A. F. Kholtygin*
Affiliation:
Astronomical Institute, St.Petersburg University, 198904 St.Petersburg, Petrodvoretz, Russia I: afx@aispbu.su

Abstract

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There are many indications for the existence of dense cold clumps in Wolf-Rayet (WR) atmospheres, expanding outwards from the stellar core (e.g., Cherepaschuck et al. 1984, St-Louis et al. 1993). Based on this, we consider a clump model for WR model atmospheres. The main features of the model are described. The mechanism of clump structure formation is outlined. The clump model is used for calculating emission line profiles.

Keywords

stars: Wolf-Rayetatmospheresinhomogeneityline profiles
Type
Session II - Model atmospheres for single Wolf-Rayet stars
Information
Symposium - International Astronomical Union , Volume 163: Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution , 1995 , pp. 160 - 161
Copyright
Copyright © Kluwer 1995 

References

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