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Physical Properties and Abundances of Novae in the Nebular Phase

Published online by Cambridge University Press:  12 April 2016

M.A.J. Snijders
M.A.J. Snijders*
Affiliation:
Astronomisches Institut Tübingen

Abstract

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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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