Hostname: page-component-7bb8b95d7b-s9k8s Total loading time: 0 Render date: 2024-09-11T17:53:19.460Z Has data issue: false hasContentIssue false
  • English
  • Français

Non-thermal velocities in the stellar wind of early-type stars

Published online by Cambridge University Press:  26 May 2016

R. de Vos  and
R. Blomme
R. de Vos
Affiliation:
IH-CTL-Gent, Voskenslaan 270, B-9000 Gent, Belgium
R. Blomme
Affiliation:
Royal Observatory of Belgium, Ringlaan 3, B-1180 Brussels, Belgium

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Turbulence is known to be important in the stellar wind of early-type stars. We explore the influence of turbulence that depends on the distance to the star.

Type
7. OB Stellar Winds
Information
Symposium - International Astronomical Union , Volume 162: Pulsation, Rotation and Mass Loss in Early-Type Stars , 1994 , pp. 498 - 499
Copyright
Copyright © Kluwer 1994 

References

Groenewegen, M.A.T., Lamers, H.J.G.L.M.: 1989, A&AS 79, 359 Google Scholar
Lamers, H.J.G.L.M., Cerruti-Sola, M., Perinotto, M.: 1987, ApJ 314, 726 CrossRefGoogle Scholar
Owocki, S.P., Castor, J.I., Rybicki, G.B.: 1988, ApJ 335, 914 CrossRefGoogle Scholar