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Radio Emission from Close Binary Systems and Novae

Published online by Cambridge University Press:  12 April 2016

R.M. Hjellming
R.M. Hjellming*
Affiliation:
National Radio Astronomy Observatory, Socorro, New Mexico, 87801, U.S.A.

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This review of the radio emission properties of close binary systems and novae will be partly concerned with surveying the star systems that exhibit continuum radio emission, and partly concerned with discussing the implications of the observed radio emission. The phenomena we will encounter will range from purely thermal continuum radio emission for the case of ionized nova shells to strong, non-thermal continuum radio emission produced by relativistic particles in both ‘normal’ and X-ray emitting close binary systems. In keeping with the subject of this symposium, let me emphasize that all regions involving radio emission are from the portions of the stellar environment where Ne ≤ 1010cm-3, generally rather high in the stellar or systemic atmosphere; however, events more closely associated with the stars themselves are the root causes of the phenomena, supplying energy, mass, magnetic fields, and relativistic particles.

Type
Part II: Cataclysmic Variables
Information
International Astronomical Union Colloquium , Volume 42: The Interaction of Variable Stars with their Environment , 1977 , pp. 279 - 291
Copyright
Copyright © Veröff. Der Remeis-Sterwarte 1977

References

Altenhoff, W.J., Braes, L.L.E., Olnon, F.M., Wendker, H.J. 1976, Astron. and Astrophys., 46, 11.Google Scholar
Altenhoff, W.J. and Wendker, H.J. 1973, Nature, 241, 37.Google Scholar
Baldwin, et. al. 1975, 1973, Nature, 241, 38.Google Scholar
Bath, G.T. and Wallerstein, G. 1975, P.A.S.P., 88, 759.Google Scholar
Brown, R.L. et. al. 1976, M.N.R.A.S., 175, 87P.Google Scholar
Clark, B.G., Kellermann, K.I., and Shaffer, D. 1975, Astrophy. J., 198, L123.Google Scholar
Clark, T.A., Button, L.K., Ma, C., Webster, W., Hinteregger, C.A., Knight, C.A., Rogers, A.E.E., Whitney, A.E., Shapiro, I.I., Wittels, J.J., Niell, A.E., and Resch, G.M. 1976, Astrophy. J., 206, L107.Google Scholar
Feldman, P.A. 1977, IAU Symposium on Planetary Nebulae, Ithaca, N.Y. Google Scholar
Gibson, D.M. 1975, Ph.D. thesis, U. of Virginia.Google Scholar
Gibson, D.M. 1977 (in preparation).Google Scholar
Gibson, D.M. and Hjellming, R.M. 1974, P.A.S.P., 86, 652.Google Scholar
Gibson, D.M., Hjellming, R.M., and Owen, F.N. 1975a, Astrophy. J., 200, L99.Google Scholar
Gibson, D.M., Hjellming, R.M., and Owen, F.N. 1975b, IAU Circ. No. 2789.Google Scholar
Gregory, P.C. and Seaquist, E.R. 1974, Nature, 247, 532.Google Scholar
Gregory, P.C., Kwok, S., and Seaquist, E.R. 1977, Ap.J., 211, 429.Google Scholar
Hall, D. 1973, private communication.Google Scholar
Hall, D. 1975, IAU Colloq. No. 29 (in press).CrossRefGoogle Scholar
Hjellming, R.M. 1972, Nature Phy. Sci., 238, 52.Google Scholar
Hjellming, R.M. 1973, Science, 182, 1089.Google Scholar
Hjellming, R.M. 1975, “Physics of Non-Thermal Radio Sources”, ed. Setti, G. (Dordrecht: Reidel), p. 203.Google Scholar
Hjellming, R.M. 1978, Astron. J. (to be submitted).Google Scholar
Hjellming, R.M. and Blankenship, L.C. 1973, Nature Phy. Sci., 243, 81.Google Scholar
Hjellming, R.M., Blankenship, L.C., and Balick, B. 1973, Nature Phy. Sci., 242, 84.Google Scholar
Hjellming, R.M. and Wade, C.M. 1970, Ap. J. (Letters), 162, L1.Google Scholar
Hjellming, R.M. and Wade, C.M. 1971, Astrophy. J., 168, L115.Google Scholar
Hjellming, R.M. and Wade, C.M. 1973, Nature, 242, 250.Google Scholar
Marsh, K.A., Purton, C.R., Feldman, P.A. 1976, Astron. and Astrophys., 49, 211.Google Scholar
Owen, F.N., Balonek, T.J., Dickel, J., Terzian, Y., and Gottesmann, S.T., 1976, Astrophy. J., 203, L15.Google Scholar
Owen, F.N. and Gibson, D.M. 1978 (in preparation).Google Scholar
Owen, F.N., Jones, T.W., and Gibson, D.M. 1977, Astrophy. J., 210, L27.Google Scholar
Panagia, N. and Felli, M. 1975, Astron. Ap., 39, 1.Google Scholar
Pooley, G.G. and Ryle, M. 1973, Nature, 244, 270.Google Scholar
Seaquist, E.R., 1976, Astrophy. J., 203, L35.Google Scholar
Schnopper, H.W., Delvaille, J.P., Epstein, A., Helmken, H., Murray, S.S., Clark, G., Jernigan, G., and Doxsey, R. 1976, Astrophys. J., 210, L75.Google Scholar
Spangler, S.R., Owen, F.N., and Hulse, R.A. 1978, A.J, (in press).Google Scholar
Spencer, J.H. and Schwartz, P.R. 1974, Astrophy. J., 188, L105.Google Scholar
Wade, C.M. and Hjellming, R.M. 1972, Nature, 235, 270.Google Scholar
Wendker, H.J., Baars, J.W.M., and Altenhoff, W.J. 1973, Nature Phy. Sci., 245, 118.Google Scholar
Wright, A.E. and Barlow, M.J., 1975, M.N.R.A.S., 170, 41.CrossRefGoogle Scholar