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Non Uniformity Expected in Nova Ejection

Published online by Cambridge University Press:  12 April 2016

M. Friedjung
M. Friedjung*
Affiliation:
Institut d’Astrophysique de paris – C.N.R.S., 98 Bis Bd Arago F 75014Paris

Extract

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It is shown that according to the model of continued ejection of nova envelopes by radiation pressure, discrete clouds are probably formed. Their properties are discussed.

Type
Part II: Cataclysmic Variables
Information
International Astronomical Union Colloquium , Volume 42: The Interaction of Variable Stars with their Environment , 1977 , pp. 322 - 326
Copyright
Copyright © Veröff. Der Remeis-Sterwarte 1977

References

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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.: 1974, in “Variable Stars and Stellar Evolution” ed. Sherwood, and Plaut, , IAU Symp. 67, p.335 Google Scholar
Frieajung, M.: 1977, in “Novae and Related Stars” Ed. Friedjung, , Reidel, Dordrecht, p. 61 Google Scholar
Shaviv, G.: 1977, in “Novae and Related Stars” Ed. Friedjung, , Reidel, Dordrecht, p. 223 Google Scholar