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The continuum energy distribution of single galactic Wolf-Rayet stars

Published online by Cambridge University Press:  25 May 2016

Bas A. den Hond ,
Peter S. Conti  and
H. Lamers
Bas A. den Hond
Affiliation:
Astronomical Institute, Utrecht University, the Netherlands
Peter S. Conti
Affiliation:
JILA, University of Colorado, Boulder CO, USA
H. Lamers
Affiliation:
Astronomical Institute, Utrecht University, the Netherlands

Abstract

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For eleven single galactic WR stars, the continuum energy distribution from the UV to the radio was obtained from literature data. Although a power law with α = 2.79 could describe all the distributions, there appear to be deviations that depend on stellar type.

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. 67 - 68
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

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