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Thermal instability in the wind of Wolf-Rayet stars

Published online by Cambridge University Press:  25 May 2016

Denise R. Gonçalves
Affiliation:
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
Vera Jatenco-Pereira
Affiliation:
Universidade de São Paulo, Instituto Astronômico e Geofísico, Av. Miguel Stéfano, 4200, 04301-904, São Paulo, Brazil
Reuven Opher
Affiliation:
Universidade de São Paulo, Instituto Astronômico e Geofísico, Av. Miguel Stéfano, 4200, 04301-904, São Paulo, Brazil

Abstract

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In this study, we investigate the formation of clumps at the base of the wind of early-type stars via thermal instability in the presence of Alfvén wave heating. As a result we show the existence of two stable equilibrium regions, one at high temperature, the diffuse medium, and another at low temperature, the clumps. We show that the two stable equilibrium regions can coexist over a narrow range of pressures describing the diffuse medium and the clumps.

Type
Part 2. Models for single star evolution of massive stars: wind + atmosphere + interior
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

dos Santos, L.C., Jatenco-Pereira, V., Opher, R. 1993, ApJ 410, 732 Google Scholar
Gonçalves, D.R., Jatenco-Pereira, V., Opher, R. 1998, ApJ 501, 797 Google Scholar
van der Hucht, K.A. 1992, The A&A Rev 4, 123 Google Scholar
Mathews, W.G., Doane, J.S. 1990, ApJ 352, 423 Google Scholar
Owocki, S.P. 1994, in: Moffat, A.F.J., Owocki, S. P., Fullerton, A. W. & St-Louis, N. (eds.), Instability and Variability of Hot-Star Winds, Proc. Isle-aux-Coudres Workshop 1993, ApSS 221, 3 Google Scholar