Hostname: page-component-78c5997874-m6dg7 Total loading time: 0 Render date: 2024-11-02T20:37:30.970Z Has data issue: false hasContentIssue false
  • English
  • Français

Radio Imaging of Symbiotic Stars

Published online by Cambridge University Press:  12 April 2016

A.R. Taylor
A.R. Taylor*
Affiliation:
Department of Physics, University of Calgary Calgary, Alberta, Canada

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.

A brief review of radio observations of individual symbiotic stars is presented, with emphasis on radio imaging of the circumstellar nebulae. The ionized nebulae are catagorized into two types: outburst ejecta and stellar winds. Among the ejecta-type there is a strong tendency for bipolar or jet morphology. In the case of the quiescent, stellar wind emitter, a few very wide binary systems (eg. Hl-36) offer the potential of directly viewing the effects of the binary interaction.

Type
Session 1. The Basic Data
Information
International Astronomical Union Colloquium , Volume 103: The Symbiotic Phenomenon , 1988 , pp. 77 - 83
Copyright
Copyright © Kluwer 1988

References

Allen, D.A. 1980, Mon. Not. Roy. astr. Soc, 192, 521.Google Scholar
Allen, D.A. 1983 Proc. Astr. Soc. Australia, 5, 211.Google Scholar
Chapman, J.M. and Cohen, R.J. 1986, Mon. Not. Roy. astr. Soc., 220, 513.Google Scholar
Chigo, F.D. and Cohen, N.L. 1981, Ap. J., 245, 988.Google Scholar
Hjellming, R.M. and Newell, R.T. 1983, Ap. J., 275, 704.Google Scholar
Hjellming, R.M. 1985 in Radio Stars, eds. Hjellming, R.M. and Gibson, D., Dordrecht: Reidel, p. 97.CrossRefGoogle Scholar
Hjellming, R.M.. van Gorkum, J.H., Taylor, A.R., Seaquist, E.R., Padin, S., Davis, R.J. and Bode, M.F. 1986 Ap. J. Letters, 305, L71.CrossRefGoogle Scholar
Hollis, J.M., Kafatos, M., Michalitsianos, A.G. and McAlister, H.A. 1985, Ap. J., 289, 765.Google Scholar
Kafatos, M., Hollis, J.M. and Michalitsianos, A.G. 1983, Ap. J. Letters, 267, L103.Google Scholar
Kafatos, M., Hollis, J.M. and Michalitsianos, A.G. 1986, Ap. J. Supp., 62, 853.Google Scholar
Kwok, S. and Purton, C.R. 1979, Ap. J., 229, 187.Google Scholar
Kwok, S., Bigneil, R.C. and Purton, C.R. 1984, Ap. J., 279, 188.CrossRefGoogle Scholar
Manchester, R.N. 1987, A. & A., 171, 205.Google Scholar
Mauron, M., Nieto, J.L., Picat, J.P., Lelievre, G. and Sol, H. 1985, A. & A. Letters, 142, L13.Google Scholar
Newell, R.T. 1981, Ph.D. Thesis, New Mexico Institute for Mining and Technology.Google Scholar
Newell, R.T. and Hjellming, R.M. Ap. J. Letters, 263, L85.Google Scholar
Porcas, R.W., Davis, R.J. and Graham, D.A. 1987, in RS Ophiuchi (1985) and the Recurrent Nova Phenomenon, ed. Bode, M.F., VNU Science Press: Utrecht, p. 203.Google Scholar
Seaquist, E.R., Taylor, A.R. and Button, S. 1984 Ap. J., 284, 202.Google Scholar
Seaquist, E.R. and Taylor, A.R. 1987, Ap. J., 312, 813.Google Scholar
Solf, J. and Ulrich, H. 1985 A. & A., 148, 274.Google Scholar
Sopka, R.J., Herbig, G., Kafatos, M. and Michalitsianos, A.G. 1982, Ap. J. Letters, 258, L35.Google Scholar
Taylor, A.R. and Seaquist, E.R. 1984, Ap. J., 286, 263.Google Scholar
Taylor, A.R., Seaquist, E.R. and Mattei, 1986, Nature, 319, 38.Google Scholar
Taylor, A.R., Davis, R.J., Porcas, R.W. and Bode, M.F. 1987, Mon. Not. Roy. Astr. Soc, submitted.Google Scholar
Wright, A.E. and Barlow, M.J. 1975, Mon. Not. Roy. astr. Soc., 170, 41.Google Scholar