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Physical Properties and Abundances of Novae in the Nebular Phase
Published online by Cambridge University Press: 12 April 2016
Abstract
We discuss the derivation and behaviour of temperatures and densities of nova ejecta during the nebular stage. A systematic comparison is made between fairly complete sets of abundances for 3 C/O and 2 Neon novae. The abundances in the ejecta might influence the formation and composition of circumstellar dust in novae.
- Type
- 1c. Nebular Ejecta
- Information
- International Astronomical Union Colloquium , Volume 122: Physics of Classical Novae , 1990 , pp. 188 - 194
- Copyright
- Copyright © Springer-Verlag 1990
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