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Towards a Realistic Model for Nova Envelopes

Published online by Cambridge University Press:  14 August 2015

M. Friedjung
M. Friedjung*
Affiliation:
Institut d'Astrophysique, Paris

Abstract

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Arguments are given, suggesting that the most probable type of model is one in which ejection continues after maximum light in the visual region, but with rapid time variations.

Type
Part 6 / Novae
Information
Symposium - International Astronomical Union , Volume 67: Variable Stars and Stellar Evolution , 1975 , pp. 335 - 338
Copyright
Copyright © Reidel 1975 

References

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