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Wolf-Rayet Binaries: Observational Aspects
Published online by Cambridge University Press: 03 August 2017
Abstract
New data concerning observational aspects of Wolf-Rayet binaries are summarised. WR+O and WR+c binary systems are considered. All the data concerning WR binaries agree well with the modern understanding of WR stars as the helium remnants formed as a result of mass loss by massive O-type stars.
- Type
- Session IV. Binaries
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- Copyright © Kluwer 1991