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Modelling the Wind Eclipses in WR+O Binaries: The Qualitative Picture

Published online by Cambridge University Press:  03 August 2017

Gloria Koenigsberger  and
Lawrence H. Auer
Gloria Koenigsberger
Affiliation:
Instituto de Astronomía, UNAM
Lawrence H. Auer
Affiliation:
Los Alamos National Laboratory, Los Alamos, NM

Abstract

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The phase dependent profile variations due to wind eclipses in WR + O binary systems are shown to be a means of establishing the WR wind structure. The results of two model calculations are presented which indicate that there are important qualitative differences between the profile variatons which will be observed in slowly -and rapidly- accelerating winds.

Type
Session III. Intrinsic Variability
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 175 - 178
Copyright
Copyright © Kluwer 1991 

References

REFERENCES

Hillier, J.D. 1988, Ap. J., 327, 822.Google Scholar
Hummer, D. 1990, private communication.Google Scholar
Khaliullin, Kh. and Cherepashchuk, A.M. 1976, Soviet Astron., 20, 186.Google Scholar
Koenigsberger, G. 1990, Astro. Astrof. in press.Google Scholar
Koenigsberger, G. and Auer, L.H. 1985, Ap. J., 297, 255.CrossRefGoogle Scholar
Munch, G. 1950, Ap. J., 112, 266.CrossRefGoogle Scholar
Schmutz, W. and Hamman, W.-R., Wessolowski, V. 1989, Astron. Astrof., 210. 236.Google Scholar