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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

Moffat, A.F.J., Vogt, N., Paquin, G., Lamontagne, R., Barrera, L.H. 1986, AJ 91, 1386 Google Scholar
Pike, C.D., Stickland, D.J., Willis, A.J., 1983, Observatory 103, 154 Google Scholar
Schmutz, W., Schweickhardt, J., Stahl, O., Wolf, B., Dumm, Th., Gäng, Th., Jankovics, I., Kaufer, A., Lehmann, H., Mandel, H., Peitz, J., Rivinius, Th. 1997, A&A 328, 219 Google Scholar
Stickland, D.J., Lloyd, C. 1990, Observatory 110, 1 Google Scholar