Hostname: page-component-76fb5796d-r6qrq Total loading time: 0 Render date: 2024-04-25T11:26:36.292Z Has data issue: false hasContentIssue false
  • English
  • Français

The Origin of the RS CVn Binaries

Published online by Cambridge University Press:  14 August 2015

P. Biermann  and
D. S. Hall
P. Biermann
Affiliation:
Astronomisches Institut, Universität Bonn, Bonn, F.R.G.
D. S. Hall
Affiliation:
Dyer Observatory, Vanderbilt University, Nashville, Tenn. U.S.A.

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.

We consider six possible origins for the RS CVn binaries based on the following possibilities. RS CVn binaries might now be either pre-main-sequence or post-main-sequence. A pre-main-sequence binary might not always have been a binary but might have resulted from fission of a rapidly rotating single pre-main-sequence star. The main-sequence counterparts might be either single stars or binaries.

To decide which of the six origins is possible, we consider the following observed data for the RS CVn binaries: total mass, total angular momentum, lack of observed connection with regions of star formation, large space density, kinematical age, and the visual companion of WW Dra. In addition we consider lifetimes and space densities of single stars and other types of binaries.

The only origin possible is that the RS CVn binaries are in a thermal phase following fission of a main-sequence single star. In this explanation the single star had a rapidly rotating core which became unstable due to the core contraction which made it begin to evolve off the main sequence. The present Be stars might be examples of such parent single stars.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 73: Structure and Evolution of Close Binary Systems , 1976 , pp. 381 - 387
Copyright
Copyright © Reidel 1976 

References

Atkins, H. L. and Hall, D. S.: 1972, Publ. Astron. Soc. Pacific 84, 638.Google Scholar
Barnes, R. C.: 1974, Publ. Astron. Soc. Pacific 86, 195.Google Scholar
Biermann, P. and Tinsley, B. M.: 1974, Astron. Astrophys. 30, 1.Google Scholar
Bodenheimer, P. and Ostriker, J. P.: 1970, Astrophys. J. 161, 1101.CrossRefGoogle Scholar
Catalano, S. and Rodono, M.: 1967, Mem. Soc. Astron. Italiana 38, 395.Google Scholar
Conti, P. S.: 1967, Astrophys. J. 149, 629.CrossRefGoogle Scholar
Delhaye, J.: 1965, in Blaauw, A. and Schmidt, M. (eds), Galactic Structure , University of Chicago Press, p. 61.Google Scholar
Dworak, T. Z.: 1973, IAU Inform. Bull. Var. Stars No. 846.Google Scholar
Field, J. V.: 1969, Monthly Notices Roy. Astron. Soc. 144, 419.Google Scholar
Fricke, K. J.: 1968, Z. Astrophys. 68, 317.Google Scholar
Fricke, K. J. and Kippenhahn, R.: 1972, Ann. Rev. Astron. Astrophys. 10, 45.Google Scholar
Goldreich, P. and Schubert, G.: 1967, Astrophys. J. 150, 571.Google Scholar
Hall, D. S.: 1968, Publ. Astron. Soc. Pacific 80, 477.Google Scholar
Hall, D. S.: 1972, Publ. Astron. Soc. Pacific 84, 323.Google Scholar
Hall, D. S.: 1974, Acta Astron. 24, 215.Google Scholar
Hall, D. S.: 1975b, Acta Astron. (submitted).Google Scholar
Hall, D. S.: 1975a, Proc. IAU Colloq. No. 29 (in preparation).Google Scholar
Huang, S. S.: 1973, Bull. Am. Astron. Soc. 5, 41.Google Scholar
James, R. A. and Kahn, F. D.: 1970, Astron. Astrophys. 5, 232.Google Scholar
James, R. A. and Kahn, F. D.: 1971, Astron. Astrophys. 12, 332.Google Scholar
Kippenhahn, R.: 1969, Astron. Astrophys. 2, 309.Google Scholar
Kippenhahn, R., Meyer-Hoffmeister, E., and Thomas, H. C.: 1970, Astron. Astrophys. 5, 155.Google Scholar
Koch, R. H., Sobieski, S., and Wood, F. B.: 1963, Publ. Univ. Pennsylvania 9.Google Scholar
Kraft, R. P.: 1967, Publ. Astron. Soc. Pacific 79, 395.Google Scholar
Montle, R. E.: 1973, , .Google Scholar
Oliver, J. P.: 1974, , .Google Scholar
Plavec, M. and Grygar, J.: 1965, Kleine Veroeffentl. Remeis Sternw. Bamberg 4, No. 40, 213.Google Scholar
Roxburgh, I. W.: 1966a, Astron. J. 71, 133.Google Scholar
Roxburgh, I. W.: 1966b, Astrophys. J. 143, 111.Google Scholar
Ulrich, R. K. and Popper, D. M.: 1974, Bull. Am. Astron. Soc. 6, 461.Google Scholar
Wielen, R.: 1974, in Coutopoulos, G. (ed.), Highlights of Astronomy , Vol. 3, D. Reidel, Dordrecht, p. 395.Google Scholar