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A search for spectral variability in WR1
Published online by Cambridge University Press: 07 August 2017
Abstract
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Preliminary results of spectroscopic monitoring of the WN5-B star WR1 (HD 4004) are presented, showing evidence for a 0d.775 period.
- Type
- Session I - Basic parameters, properties of single Wolf-Ray et stars
- Information
- Copyright
- Copyright © Kluwer 1995
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