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Clumps and shocks in the outer winds of hot stars

Published online by Cambridge University Press:  26 May 2016

Mark C. Runacres  and
Stanley P. Owocki
Mark C. Runacres
Affiliation:
Koninklijke Sterrenwacht, Ringlaan 3, B-1180 Brussel, België
Stanley P. Owocki
Affiliation:
Bartol Research Institute, University of Delaware, Newark, DE 19716, USA

Abstract

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We present a moving periodic box technique to study the outer-wind evolution of instability-generated structure in hot-star winds. This has considerable computational and conceptual advantages

Type
Part 1. Atmospheres of Massive Stars
Information
Symposium - International Astronomical Union , Volume 212: A Massive Star Odyssey: From Main Sequence to Supernova , 2003 , pp. 226 - 227
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Runacres, M.C., Owocki, S.P. 2002, A&A 381, 1015.Google Scholar