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The IUE orbit of γ2 Velorum

Published online by Cambridge University Press:  25 May 2016

Chris Lloyd  and
David J. Stickland
Chris Lloyd
Affiliation:
Space Science Department, Rutherford Appleton Laboratory, Chilton, Didcot, Oxon OX11 0QX, UK
David J. Stickland
Affiliation:
Space Science Department, Rutherford Appleton Laboratory, Chilton, Didcot, Oxon OX11 0QX, UK

Abstract

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Using IUE-SWP spectra, an orbital solution is derived for both components in the γ2 Velorum, which supports the lower mass of the O star found previously.

Type
Part 3. Interaction of Wolf-Rayet stars and other hot massive stars with their environment: colliding winds and ring nebulae
Information
Symposium - International Astronomical Union , Volume 193: Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies , 1999 , pp. 364 - 365
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

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Stickland, D.J., Lloyd, C. 1990, Observatory 110, 1 Google Scholar