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FUSE1 observations of stellar wind variability in the LMC supergiant Sk–67°166 (O4 If+)

Published online by Cambridge University Press:  26 May 2016

Alexander W. Fullerton ,
Derck L. Massa ,
Raman K. Prinja ,
Ian D. Howarth ,
Allan J. Willis  and
Stanley P. Owocki
Alexander W. Fullerton
Affiliation:
Department of Physics and Astronomy, University of Victoria, PO Box 3055, Victoria, BC V8W 3P6, Canada Department of Physics and Astronomy, The Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218, USA
Derck L. Massa
Affiliation:
SGT Inc., NASA's Goddard Space Flight Center, Code 681.0, Greenbelt, MD 20771, USA
Raman K. Prinja
Affiliation:
Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, UK
Ian D. Howarth
Affiliation:
Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, UK
Allan J. Willis
Affiliation:
Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, UK
Stanley P. Owocki
Affiliation:
Bartol Research Institute, University of Delaware, Newark, DE 19716, USA

Abstract

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We describe FUSE time-series observations of stellar wind variability in Sk-67°166 (HDE 269698), a nitrogen-rich O4 supergiant in the LMC.

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. 182 - 183
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Shanow, D.J., Moos, H.W., Ake, T.B., et al. 2000, ApJ (Letters) 538, 7.Google Scholar