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Observational Effects of Corotating Interaction Regions in OB stars

Published online by Cambridge University Press:  26 May 2016

R. Blomme
R. Blomme*
Affiliation:
Royal Observatory of Belgium, Ringlaan 3, B-1180 Brussel, Belgium

Abstract

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The stellar winds of OB stars are perturbed by Corotating Interaction Regions (CIRs). We present a 3D radiative transfer model which predicts that variations should occur in the infrared and millimetre continuum.

Type
Session 1 Observations of Rotating Stars
Information
Symposium - International Astronomical Union , Volume 215: Stellar Rotation , 2004 , pp. 47 - 48
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

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