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Formation of Ring Nebulae around Massive Stars in LMC HII Regions

Published online by Cambridge University Press:  25 May 2016

Kerstin Weis  and
Wolfgang J. Duschl
Kerstin Weis
Affiliation:
ITA, Univ. Heidelberg, Tiergartenstr. 15, 69121 Heidelberg, Germany Astronomy Department, University of Illinois, Urbana, IL 61801, USA
Wolfgang J. Duschl
Affiliation:
ITA, Univ. Heidelberg, Tiergartenstr. 15, 69121 Heidelberg, Germany MPI für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany

Abstract

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Massive stars have strong stellar winds and consequently a high mass loss during their lifetimes. Therefore they can form ring nebulae by stellar winds sweeping up the ambient medium in the main sequence phase or through wind-wind interaction or eruptions in the evolved state. We present preliminary results of a search for single bubbles and ring-nebulae around massive stars in the Large Magellanic Cloud (LMC).

Type
Part 2. Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 134 - 135
Copyright
Copyright © Astronomical Society of the Pacific 1999