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A Survey of Nova Remnants*

Published online by Cambridge University Press:  12 April 2016

H.W. Duerbeck  and
W.C. Seitter
H.W. Duerbeck
Affiliation:
Astronomisches Institut Universität Münster, Münster, F.R.G.
W.C. Seitter
Affiliation:
Astronomisches Institut Universität Münster, Münster, F.R.G.

Abstract

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Exnovae and nova shells are generally faint and difficult to observe. Only a few have been studied, and even less of them in sufficient detail. We give a progress report on our survey of exnovae and nova shells, especially on the results of a spectral survey of novae in the southern Milky Way. The three-dimensional structure in the light of Hα derived for the nebula of GK Per is displayed.

Type
V. Nova and Dwarf Nova Outbursts
Information
International Astronomical Union Colloquium , Volume 93: Cataclysmic Variables: Recent Multi-Frequency Observations and Theoretical Developments , 1987 , pp. 467 - 473
Copyright
Copyright © Reidel 1987

Footnotes

Based on observations obtained at the European Southern Observatory, La Silla, Chile, and at the Centro Astronomico Hispano-Aleman Calar Alto, Spain, operated by the Max-Planck-Institut für Astronomie, Heidelberg.

References

Duerbeck, H.W. 1986, Space Sci. Rev. (submitted).Google Scholar