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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.

Information

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

Claudi, R.U., Cremonese, G. 1993, Asiago and Padova Observatories Handbook Google Scholar
Helfand, D.J. 1980, PASP 92, 691 CrossRefGoogle Scholar
Lamontagne, R. 1983, PhD thesis, Université de Montréal Google Scholar
Moffat, A.F.J., Shara, M.M. 1986, AJ 92, 952 CrossRefGoogle Scholar
Robert, C. et al. 1992, ApJ 397, 277 CrossRefGoogle Scholar