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Wolf-Rayet stars in OB associations

Published online by Cambridge University Press:  25 May 2016

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

Abstract

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We present first results of our search for Wolf-Rayet members of OB associations, aiming in determination of distances and absolute magnitudes for WR stars.

Type
Part 1. Basic observational properties of Wolf-Rayet stars and other hot massive stars
Information
Symposium - International Astronomical Union , Volume 193: Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies , 1999 , pp. 82 - 83
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Garmany, C.D., Stencel, R.E. 1992, A&AS 94, 211 Google Scholar
van der Hucht, K.A., Schrijver, H., Stenholm, B., Lundström, I., Moffat, A.F.J., Seggewiss, W., Setia Gunawan, D.Y.A., Sutantyo, W., van den Heuvel, E.P.J., De Cuyper, J.-P., Gómez, A., Marchenko, S.V. 1997, New Astronomy 2, 245 Google Scholar
van der Hucht, K.A. 1999, in preparation Google Scholar
Lundström, I., Stenholm, B. 1984, A&AS 58, 163 Google Scholar
Melnik, A.M., Efremov, Y.N. 1995, PAZ 21, 13 Google Scholar