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The stellar parameters of the SMC WR binary HD 5980

Published online by Cambridge University Press:  25 May 2016

Jörg Schweickhardt  and
Werner Schmutz
Jörg Schweickhardt
Affiliation:
Landessternwarte Königstuhl, D-69117 Heidelberg, Germany
Werner Schmutz
Affiliation:
Institut für Astronomie, ETH-Zentrum, CH-8092 Zürich, Switzerland

Abstract

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We present the temporal variation of the stellar parameters of the erupting star in HD 5980. We derive the effective temperature and radius from the observed changes of the visual magnitude. Our analysis is based on the assumption that the luminosity of the erupting star remained constant and that the brightness of the second star did not vary.

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. 101 - 102
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Jones, A., Sterken, C. 1997, J. Astron. Data 3, 4 Google Scholar
Koenigsberger, G., Peña, M., Schmutz, W., Ayala, S. 1998, ApJ 499, 889 CrossRefGoogle Scholar
Sterken, C., Breysacher, J. 1997, A&A 328, 269 Google Scholar