Hostname: page-component-5c6d5d7d68-vt8vv Total loading time: 0.001 Render date: 2024-08-17T10:14:49.289Z Has data issue: false hasContentIssue false
  • English
  • Français

Algols: Wherefrom, Whereto, and What in Between ?

Published online by Cambridge University Press:  12 April 2016

J. P. De Greve
J. P. De Greve*
Affiliation:
Astrophysical Institute,V.U.B. Pleinlaan 2, B 1050 Brussels,Belgium

Abstract.

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Four different aspects related to the evolution of Algols are discussed: the occurrence of a contact phase during the mass transfer, the evolution of short period systems evolving through case A mass transfer, the influence of the mass transfer on the surface abundances of both components, and the problem of the initial parameters of Algol systems. For the latter, a search is made for conservative case B systems. UZ Cyg seems to be a good candidate for such evolution. Finally, some remarks are given on the initial values of the low mass Algol S Cancri.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 107: Algols , 1989 , pp. 127 - 139
Copyright
Copyright © Kluwer 1989

References

Andersen, J., Clausen, J.V., Gustafsson, B., Nordstrom, B., Vandenberg, D.A.: 1988, Astron. Astrophys. (in press)Google Scholar
Awadalla, N.S., Budding, E.: 1982, in Kopal, Z. and Rahe, J. (eds.) ‘Binary and Multiple Stars as Tracers of Stellar Evolution Theory’, D. Reidel Publ. Co., Dordrecht, Holland, p.239.Google Scholar
Batten, A.H., Tomkin, J.: 1984, Astrophys. J. 285, 208.Google Scholar
Benson, R.S.: 1970, Ph. D. thesis, Univ. of California, Berkeley.Google Scholar
Cugier, H., Hardorp, J.: 1988, Astron. Astrophys. (in press).Google Scholar
De Greve, J.P.: 1980, Astrophys. Space Sci. 73, 411.Google Scholar
De Greve, J.P.: 1986, Space Science Rev. 43, 139.Google Scholar
De Greve, J.P., de Landtsheer, A.C., Packet, W.: 1984, Astron. Astrophys. 142, 367.Google Scholar
De Greve, J.P., Cugier, H.: 1988, Astron. Astrophys. (in press).Google Scholar
Dobias, J.J.: 1985, Ph. D. thesis, UCLA, Los Angeles.Google Scholar
Giuricin, G., Mardirossian, F., Mezzetti, M.: 1983, Astrophys. J. Suppl. Ser. 52, 35.Google Scholar
Lucy, L.B., Wilson, R.E.: 1979, Astrophys. J. 231, 502.Google Scholar
Nakamura, M., Nakamura, Y.: 1982, Astrophys. Space Sci. 83, 163.Google Scholar
Nakamura, M., Nakamura, Y.: 1984, Astrophys. Space Sci. 104, 367.Google Scholar
Nakamura, M., Nakamura, Y.: 1987a, Astrophys. Space Sci. 134, 161.CrossRefGoogle Scholar
Nakamura, M., Nakamura, Y.: 1987b, Astrophys. Space Sci. 134, 219.Google Scholar
Packet, W.: 1988, Ph. D. thesis, V.U.B., Brussels.Google Scholar
Paczynski, B.: 1976, in Eggleton, P. et al. (eds.) ‘Structure and Evolution of Close Binary Systems’, D.Reidel Publ. Co., Dordrecht, Holland, p.75.Google Scholar
Partasarathy, M., Lambert, D.L., Tomkin, J.: 1983, Monthly Not. Roy. Astron. Soc. 203, 1063.Google Scholar
Plavec, M.J.: 1973, in Batten, A.H. (ed.), ‘Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems’, D. Reidel Publ. Co., Dordrecht, Holland, p.216.Google Scholar
Refsdal, S., Roth, M.L., Weigert, A.: 1974, Astron. Astrophys. 36, 113.Google Scholar
Rucinski, S.M.: 1974, Acta Astron. 24, 119.Google Scholar
Rucinski, S.M.: 1976, Publ. Astron. Soc. Pacific 88, 244.Google Scholar
Smith, R.C.: 1884, Quart. J. Roy. Astron. Soc. 25, 405.Google Scholar
van’t Veer, F.: 1979, Astron. Astrophys. 80, 287.Google Scholar
Webbink, R.F.: 1976, Astrophys. J. Suppl. Ser. 32, 583.Google Scholar
Webbink, R.F.: 1980, in Plavec, M.J. et al. (eds.) ‘Close Binary Stars: Observations and Interpretation’, D.Reidel Publ. Co., Dordrecht, Holland, p.127.Google Scholar