Abstract
In this paper we show that for eight components of early type binary systems (including three supergiants) the orbital mass corresponds reasonably well with masses resulting from evolutionary computations.
This is a preview of subscription content, log in via an institution to check access.
References
Hubeny, I., 1988, Comp. Phys. Comm. 52, 103.
Joss, P.C., Rappaport, S.A., 1984, Ann. Rev. Astron. Astrophys. 22, 537.
Kudritzki, R.P. and Hummer, D.G., 1986, in Luminous Stars and Associations in Galaxies, editors C.W.H. De Loore et al.
Kurucz, 1991, private communication.
Maeder, A.,1991, Astron. Astrophys. (in press).
Popper, D.M., 1980, Ann. Rev. Astron. Astrophys. 18, 115.
Vanbeveren, D.: 1990, Astron. Astrophys. 234, 243.
Author information
Authors and Affiliations
Editor information
Rights and permissions
Copyright information
© 1992 Springer-Verlag
About this paper
Cite this paper
Vrancken, M., van Rensbergen, W., Vanbeveren, D. (1992). A comparison between the orbital masses of early type binary components and masses predicted by stellar evolution. In: Heber, U., Jeffery, C.S. (eds) The Atmospheres of Early-Type Stars. Lecture Notes in Physics, vol 401. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-55256-1_270
Download citation
DOI: https://doi.org/10.1007/3-540-55256-1_270
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-55256-7
Online ISBN: 978-3-540-46997-1
eBook Packages: Springer Book Archive