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Some aspects of the spectral variability of WR 141
Published online by Cambridge University Press: 25 May 2016
Abstract
An analysis of the behaviour of the He II 5411 line wings is presented. The spectral classification of the companion is discussed on the basis of a simple geometric model of the colliding stellar winds zone.
- Type
- Part 1. Basic observational properties of Wolf-Rayet stars and other hot massive stars
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- Copyright © Astronomical Society of the Pacific 1999