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Spectral variability versus radial-velocity changes in WR 1

Published online by Cambridge University Press:  25 May 2016

Andrzej Niedzielski
Andrzej Niedzielski*
Affiliation:
Toruñ Centre for Astronomy, Nicolas Copernicus University, ul. Gagarina 11, 87–100 Toruñ, Poland

Abstract

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We discuss the possibility that WR 1 (HD 4004) is a binary system.

Type
Part 2. Models for single star evolution of massive stars: wind + atmosphere + interior
Information
Symposium - International Astronomical Union , Volume 193: Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies , 1999 , pp. 254 - 255
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

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