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Effects of the Presence of Supercritical Winds

Published online by Cambridge University Press:  12 April 2016

Michael Friedjung
Michael Friedjung*
Affiliation:
Institut d’Astrophysique, 98 bis Boulevard Arago, 75014 Paris, France.

Abstract

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Evidence is given that classical novae have optically thick winds for a certain time after optical maximum. Multifrequency observations especially of FH Ser indicate acceleration of the wind at very large optical depths, probably by radiation pressure of an object above the Eddington limit. This result though fairly convincing needs checking by proper radiative transfer calculations. A way in which it might be produced is mentioned as is the influence of the wind on the structure of the ejected envelope.

Type
2. Models of Observations
Information
International Astronomical Union Colloquium , Volume 122: Physics of Classical Novae , 1990 , pp. 244 - 252
Copyright
Copyright © Springer-Verlag 1990

References

Andrade, A.A., Friedjung, M.: 1989, Astron. Astrophys. in press.Google Scholar
Bath, G.T.: 1978, Mon. Not. R. astr. Soc. 182, 35.CrossRefGoogle Scholar
Bath, G.T., Shaviv, G.: 1976, Mon. Not. R. astr. Soc. 175, 305.Google Scholar
Friedjung, M.: 1966, Mon. Not. R. astr. Soc. 132, 317.Google Scholar
Friedjung, M. 1977, in “Novae and Related Stars”, ed Friedjung, M., Reidel, Dordrecht, p. 61.CrossRefGoogle Scholar
Friedjung, M.: 1981, Acta Astron. 31, 373.Google Scholar
Friedjung, M.: 1987a, Astron. Astrophys. 179, 164.Google Scholar
Friedjung, M.: 1987b, Astron. Astrophys. 180, 155.Google Scholar
Gallagher, J.S., Code, A.D.: 1974, Astrophys. J. 189, 303.CrossRefGoogle Scholar
Geisel, S.L., Kleinmann, D.E., Low, F.J.: 1970, Astrophys. J. 161, L101.Google Scholar
Harkness, R.P.: 1983, Mon. Not. R. astr. Soc. 204, 45.CrossRefGoogle Scholar
Kato, M.: 1983, Publ. astr. Soc Japan 35, 507.Google Scholar
Kato, M.: 1985, Publ. astr. Soc. Japan 37, 19.Google Scholar
Krautter, J., Beuermann, K., Leitherer, C., Oliva, E., Moorwood, A.F.M., Deul, E., Wargau, W., Klare, G., Kohoutek, L., Van Paradijs, J., Wolf, B.: 1984, Astron.Astrophys. 137, 307.Google Scholar
MacDonald, J.: 1980, Mon. Not. R. astr. Soc. 191, 933.CrossRefGoogle Scholar
MacDonald, J., Fujimoto, M.Y., Truran, J.W.: 1985, Astrophys. J. 294, 263.Google Scholar
McLaughlin, D.B.: 1947, Publ. astr. Soc. Pacific 59, 244.Google Scholar
Ruggles, L.L.N., Bath, G.T.: 1979, Astron. Astrophys. 80, 97.Google Scholar
Shara, M.: 1989, Publ. astr. Soc. Pacifie 101, 5.CrossRefGoogle Scholar
Snijders, M.A.J., Batt, T.J., Roche, P.F., Seaton, M.J., Morton, D.C., Spoelstra, T.A.T., Blades, J.C.: 1987, Mon. Not. R. astr. Soc. 228, 329.Google Scholar
Stickland, D., Penn, C.J. Seaton, M.J., Snijders, M.A.J., Storey, P.J., Kitchin, C.R.: 1979, in “The First Year of IUE”, ed. Willis, A.J., University College, London, p. 63.Google Scholar
Stickland, D.J., Penn, C.J., Seaton, M.J., Snijders, M.A.J., Storey, P.J.: 1981. Mon. Not. R. astr. Soc. 197, 107.Google Scholar
Turolla, R., Nobili, L., Calvani, M.: 1988, Astrophys. J. 324, 899.Google Scholar
Whipple, F.L., Payne-Gaposchkin, C.: 1936, Circ astr. Obs. Harvard 413.Google Scholar