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Synthetic line profiles from unified model atmospheres

Published online by Cambridge University Press:  07 August 2017

E. Santolaya Rey ,
A. Herrero  and
J. Puls
E. Santolaya Rey
Affiliation:
Institute de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
A. Herrero
Affiliation:
Institute de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
J. Puls
Affiliation:
Institut für Astronomie und Astrophysik, Scheinerstraße 1, D-81679 München, B.R.D.

Abstract

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Synthetic line-profiles from unified model atmospheres are presented. The main characteristics of the code are also shown concerning both the calculation of NLTE populations (in a consistent way with the radiation field), and the formal solution to obtain emergent profiles. Stark-broadening is considered in this last step. Emergent Hα profiles for a grid of models are shown for Teff = 50 000 K, covering a wide range of stellar radii and mass-loss.

Keywords

stars: atmospheresearly typemass-lossradiative transferline-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. 164 - 165
Copyright
Copyright © Kluwer 1995 

References

Puls, J., Hummer, D. 1987, A&A 191, 87 Google Scholar
Hamann, W.R., Schmutz, W. 1987, A&A 174, 173 Google Scholar
Schöning, T., Butler, K. 1989, A&A 219, 362 Google Scholar