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ISO-PHOT observations of Wolf-Rayet winds

Published online by Cambridge University Press:  25 May 2016

Mark C. Runacres ,
Ronny Blomme ,
Koen Vyverman ,
Martin Cohen ,
Claus Leitherer ,
Stanley P. Owocki  and
Martin Haas
Mark C. Runacres
Affiliation:
Royal Observatory of Belgium, B-1180 Brussel, Belgium
Ronny Blomme
Affiliation:
Royal Observatory of Belgium, B-1180 Brussel, Belgium
Koen Vyverman
Affiliation:
Vrije Universiteit Brussel, B-1050 Brussel, Belgium
Martin Cohen
Affiliation:
Radio Astronomy Lab., Univ. of California, Berkeley, CA 94720, USA
Claus Leitherer
Affiliation:
Space Telescope Science Institute, Baltimore, MD 21218, USA
Stanley P. Owocki
Affiliation:
Bartol Research Institute, Univ. of Delaware, Newark, DE 19716, USA
Martin Haas
Affiliation:
Max-Planck Institut für Astronomie, D-69117 Heidelberg, Germany

Abstract

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We use ISO-PHOT maps around five WN stars to derive their far-infrared fluxes. In some cases we also detect a nebula around the star.

Type
Part 1. Basic observational properties of Wolf-Rayet stars and other hot massive stars
Information
Symposium - International Astronomical Union , Volume 193: Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies , 1999 , pp. 96 - 97
Copyright
Copyright © Astronomical Society of the Pacific 1999