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Observational study of the evolution of massive binary stars
Published online by Cambridge University Press: 04 August 2017
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Six years ago an observational program on supergiant stars using CORAVEL was initiated at Geneva Observatory. About 1500 radial velocities were obtained out of a sample of 181 northern supergiants of F, G, K, M type. Nineteen new SB have been discovered and 16 others are suspected to be SB. The total rate of binary systems among northern supergiants is in the range of 31–38 % (Burki and Mayor, 1983). This value neither depends on spectral type nor luminosity class.
- Type
- III. BINARITY, PULSATION, ROTATION AND MIXING
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- Copyright © Reidel 1984
References
Batten, A.H., Fletcher, J.M., Mann, P.J.: 1978, Publ. Dominion Astrophys. Obs.
15, 121.Google Scholar
Kopal, Z.: 1978, Dynamics of Close Binary Systems, D. Reidel, Dordrecht, Holland, p. 414.CrossRefGoogle Scholar