Hostname: page-component-7479d7b7d-pfhbr Total loading time: 0 Render date: 2024-07-12T02:03:42.389Z Has data issue: false hasContentIssue false
  • English
  • Français

Symbiotic Binary Stars

Published online by Cambridge University Press:  07 August 2017

Scott J. Kenyon
Scott J. Kenyon*
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden Street, Cambridge, MA 02138

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.

This paper briefly reviews the physical properties of symbiotic stars: long-period interacting binaries composed of a red giant primary star and a hot companion. Two types of binaries produce symbiotic optical spectra: semi-detached systems with a main sequence secondary and detached systems with a white dwarf secondary. Semi-detached symbiotics resemble cataclysmic variables and Algol binaries, but on a much larger scale, and undergo dwarf nova-like eruptions. Wind accretion powers detached systems; occasional thermonuclear runaways produce symbiotic novae - distant cousins of classical novae.

Keywords

stars: binaries: symbioticsaccretion discsstars: mass loss
Type
Invited Papers
Information
Symposium - International Astronomical Union , Volume 151: Evolutionary Processes in Interacting Binary Stars , 1992 , pp. 137 - 146
Copyright
Copyright © Kluwer 1992 

References

Allen, D.A. 1980. Mon. Not. Roy. Astr. Soc. , 190, 75.Google Scholar
Allen, D.A. 1983. Mon. Not. Roy. Astr. Soc. , 204, 113.Google Scholar
Allen, D.A. 1984. Publ. Astr. Soc. Aus. , 35, 369.CrossRefGoogle Scholar
Allen, D.A. 1988. In The Symbiotic Phenomenon , IAU Colloquium No. 103, edited by Mikolajewska, J., et al. (Kluwer, Dordrecht), p. 3.Google Scholar
Aller, L.H. 1954. In Astrophysics - Nuclear Transformations, Stellar Interiors, and Nebulae (New York: Ronald), p. 180.Google Scholar
Berman, L. 1932. Publ. Astr. Soc. Pac. , 44, 318.Google Scholar
Blanco, B.M., Blanco, V.M., and McCarthy, M.F. 1978. Nature , 271, 638.Google Scholar
Duerbeck, H.W. 1984. Astrophys. Space Sci. , 99, 363.CrossRefGoogle Scholar
Dupree, A.K. 1986. Ann. Rev. Astr. Ap. , 24, 377.Google Scholar
Duschl, W.J. 1988. In The Symbiotic Phenomenon , IAU Colloquium No. 103, edited by Mikolajewska, J., et al. (Kluwer, Dordrecht), p. 27.Google Scholar
Fleming, W.P. 1912. Ann. Harv. Coll. Obs. 56, 165.Google Scholar
Garcia, M.R., Baliunas, S.L., Doxsey, R., Elvis, M., Fabbiano, G., Koenigsberger, G., Patterson, J., Schwartz, D., Swank, J., and Watson, M.G. 1983. Astrophys. J. , 267, 291.CrossRefGoogle Scholar
Hack, M., and Selvelli, P.L. 1982. Astr. Astrophys. , 107, 200.Google Scholar
Hogg, F.S. 1934. Publ. Am. Astr. Soc. , 38, 14.Google Scholar
Iben, I. Jr., and Tutukov, A.V. 1984. Astrophys. J. Suppl. , 54, 335.CrossRefGoogle Scholar
Isliker, H., Nussbaumer, H., and Vogel, M. 1989. Astr. Astrophys. , 219, 271.Google Scholar
Kenyon, S.J. 1986. The Symbiotic Stars (Cambridge: Cambridge University Press).Google Scholar
Kenyon, S.J., Fernández-Castro, T., and Stencel, R.E. 1988. Astr. J. , 95, 1817.CrossRefGoogle Scholar
Kenyon, S.J., and Garcia, M.R. 1989. Astr. J. , 97, 194.Google Scholar
Kenyon, S.J., Oliversen, N.A., Mikolajewska, J., Mikolajewski, M., Stencel, R.E., Garcia, M.R., and Anderson, C.M. 1990. Astr. J. , 101, 637.Google Scholar
Kenyon, S.J., and Truran, J.W. 1983. Astrophys. J. , 273, 280.Google Scholar
Kenyon, S.J., and Webbink, R.F. 1984. Astrophys. J. , 279, 252.Google Scholar
Kuiper, G.P. 1941. Astrophys. J. , 93, 133.Google Scholar
Menzel, D.H. 1946. Physica , 12, 768.Google Scholar
Merrill, P.W., and Humason, M.L. 1932. Publ. Astr. Soc. Pac. , 44, 56.Google Scholar
Mikolajewska, J., Friedjung, M., Kenyon, S.J., and Viotti, R. 1988. editors, The Symbiotic Phenomenon , IAU Colloquium No. 103, (Kluwer, Dordrecht).Google Scholar
Mikolajewska, J., and Kenyon, S.J. 1992a. Astr. J , submitted.Google Scholar
Mikolajewska, J., and Kenyon, S.J. 1992b. Mon. Not. Roy. Astr. Soc. , submitted.Google Scholar
Mikolajewska, J., Kenyon, S.J., and Mikolajewski, M. 1989. Astr. J. , 98, 1427.Google Scholar
Mürset, U., Nussbaumer, H., Schmid, H.M., and Vogel, M. 1991. Astr. Astrophys., .Google Scholar
Nussbaumer, H., and Stencel, R.E. 1987. In Exploring the Universe with the IUE Satellite , edited by Kondo, Y. (Reidel, Dordrecht), p. 203.CrossRefGoogle Scholar
Nussbaumer, H., Schild, H., Schmid, H.M., and Vogel, M. 1988. Astr. Astrophys. , 198, 179.Google Scholar
Nussbaumer, H., and Vogel, M. 1987. Astr. Astrophys. , 182, 51.Google Scholar
Paczynski, B. 1976. Acta Astr. , 21, 417.Google Scholar
Payne-Gaposchkin, C. 1957. The Galactic Novae (Amsterdam: North Holland)Google Scholar
Savage, B.D., and Mathis, J.S. 1979. Ann. Rev. Astr. Ap. , 17, 73.Google Scholar
Seaquist, E.R., and Taylor, A.R. 1990, Astrophys. J. , 349, 313.Google Scholar
Tout, C.A., and Eggleton, P.P. 1988. Mon. Not. Roy. Astr. Soc. , 231, 823.Google Scholar
van den Bergh, S., and Tammann, G.A. 1991. Ann. Rev. Astr. Ap. , 29, 363.Google Scholar
Vogel, M. 1991. Astr. Astrophys., ,.Google Scholar
Wallerstein, G. 1981, Observatory , 101, 172.Google Scholar
Webster, B.L., and Allen, D.A. 1975. Mon. Not. Roy. Astr. Soc. , 171, 171.Google Scholar
Whitelock, P.A. 1987. Publ. Astr. Soc. Pac. , 99, 573.Google Scholar
Willson, L.A., Wallerstein, G., Brugel, E., and Stencel, R.E. 1984. Astr. Astrophys. , 133, 154.Google Scholar
Wood, P.R. 1973, Publ. Astr. Soc. Aus. , 2, 198.Google Scholar