Hostname: page-component-f554764f5-c4bhq Total loading time: 0 Render date: 2025-04-08T20:37:53.598Z Has data issue: false hasContentIssue false
  • English
  • Français

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

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.

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

Friedjung, M.: 1966, Monthly Notices Roy. Astron. Soc. 131, 447.CrossRefGoogle Scholar
Friedjung, M.: 1968, Astrophys. Letters 2, 121.Google Scholar
Friedjung, M. and Malakpur, I.: 1974, Astrophys. Space Sci. 25, 433.CrossRefGoogle Scholar
Gallagher, J. S. and Code, A. D.: 1974, Astrophys. J. 189, 303.CrossRefGoogle Scholar
McLaughlin, D. B.: 1964, in Novae, Novoides et Supernovae, Centre National de la Recherche Scientifique, Paris, p. 123.Google Scholar
Mustel, E. R.: 1957, in Herbig, G. H. (ed.), ‘Non-Stable Stars’, IAU Symp. 3, 57.Google Scholar
Nariai, K.: 1974, Astron. Astrophys. 36, 231.Google Scholar
Pottasch, S. R.: 1959, Ann. Astrophys. 22, 394.Google Scholar
Pottasch, S. R.: 1967, Bull. Astron. Inst. Neth. 19, 227.Google Scholar