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The continuum energy distribution of single galactic Wolf-Rayet stars
Published online by Cambridge University Press: 25 May 2016
Abstract
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
- Copyright
- Copyright © Astronomical Society of the Pacific 1999