Hostname: page-component-68945f75b7-qvshk Total loading time: 0 Render date: 2024-08-06T09:20:12.594Z Has data issue: false hasContentIssue false
  • English
  • Français

Smooth winds and clumped winds for early-type stars

Published online by Cambridge University Press:  26 May 2016

R. Blomme  and
M. Runacres
R. Blomme
Affiliation:
Royal Observatory of Belgium, Ringlaan 3, B-1180 Brussels, Belgium
M. Runacres
Affiliation:
Vrije Universiteit Brussel, Pleinlaan 2, B-1050 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.

The use of the IR and radio continuum as a clumping indicator for the stellar wind of early-type stars is investigated.

Type
7. OB Stellar Winds
Information
Symposium - International Astronomical Union , Volume 162: Pulsation, Rotation and Mass Loss in Early-Type Stars , 1994 , pp. 494 - 495
Copyright
Copyright © Kluwer 1994 

References

Lucy, L.B., Solomon, P.M.: 1970, ApJ 159, 879 Google Scholar
Owocki, S.P., Castor, J.I., Rybicki, G.B.: 1988, ApJ 335, 914 Google Scholar
Runacres, M.C., Blomme, R.: 1994, in Instability and Variability of Hot Star Winds , Kluwer, in press Google Scholar