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The mass loss rate of γ Velorum
Published online by Cambridge University Press: 14 August 2015
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The CIII λ 1909 absorption feature (deepest at V=−1600 Km s−1) in this star, observed by Burton et al (1975) and Johnson (1978), was predicted by Castor and Nussbaumer (1972). It implies a copious flow of CIII ions, because the oscillator strength is only fik = 1.6× 10−7.
- Type
- Session 5: Theory and Mass Loss Rates Binary Stars - Miscellaneous Topics
- Information
- Symposium - International Astronomical Union , Volume 83: Mass Loss and Evolution of O-Type Stars , 1979 , pp. 253 - 256
- Copyright
- Copyright © Reidel 1979
References
Burton, W.M., Evans, R.G., and Griffin, W.G.: 1975, Phil. Trans. R. Soc. London A
279, pp. 355–369.Google Scholar
Nugis, T.: 1975, in Sherwood, B. & Plaut, L. (ed), Variable Stars and Stellar Evolution, D. Reidel Co., Dordrecht, pp. 291–296.Google Scholar
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