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A search for spectral variability in WR1

Published online by Cambridge University Press:  07 August 2017

A. Niedzielski
A. Niedzielski*
Affiliation:
N. Copernicus University, ul. Chopina 12/18, 87-100 Toruń, Poland

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
Symposium - International Astronomical Union , Volume 163: Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution , 1995 , pp. 52 - 53
Copyright
Copyright © Kluwer 1995 

References

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