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Optical spectroscopic variability of possible Wolf-Rayet binaries

Published online by Cambridge University Press:  25 May 2016

Aaron Flores ,
Octavio Cardona  and
Gloria Koenigsberger
Aaron Flores
Affiliation:
Instituto Nacional de Astrofisica Optica y Electronica, Mexico
Octavio Cardona
Affiliation:
Instituto Nacional de Astrofisica Optica y Electronica, Mexico
Gloria Koenigsberger
Affiliation:
Instituto de Astronomia, UNAM, Mexico

Extract

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There are a number of Wolf-Rayet stars which, based on their emission line profile variations, were proposed to be WR+cc systems (Firmani et al. 1980; Cherepashchuk & Aslanov 1984). However, recent intensive monitoring with different observational techniques, has given rise to alternative explanations for the variability in these WR stars including the presence of a disk, rotating jet-like structures (Vreux et al. 1992), and corotating interaction regions (St-Louis et al. 1995).

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. 65 - 66
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Auer, L.H., Koenigsberger, G. 1994, ApJ 436, 859 Google Scholar
Cherepashchuk, A.M., Aslanov, A.A. 1984, ApSS 102, 97 Google Scholar
Firmani, C., Koenigsberger, G., Bisiacchi, G.F., Moffat, A.F.J. Issertedt, J. 1980, ApJ 239, 607 Google Scholar
St-Louis, N., Dalton, M.J., Marchenko, S.V., Moffat, A.F.J., Willis, A.J. 1995, ApJ 452, L57 Google Scholar
Vreux, J.-M., Gosset, E., Bohannan, B., Conti, P.S. 1992, A&A 256, 148 Google Scholar