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Typical examples of classical novaeBecause of the very complicated individualistic behavior of each nova, we think it necessary to review the observations of a few well-observed individuals. We have selected a few objects of different speed classes, which have been extensively observed. They are: V1500 Cygni 1975, a very fast nova; V603 Aql 1918, fast nova; CP Pup 1942, fast nova; GK Per 1901, fast nova; V 1668 Cyg 1979, moderately fast nova; FH Ser 1970, slow nova; DQ Her 1934, slow nova; T Aur 1891, slow nova; RR Pic 1925, slow nova; and HR Del 1967, very slow nova.
Document ID
19950020654
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Hack, Margherita (Osservatorio Astronomico Trieste, Italy)
Selvelli, Pierluigi (Osservatorio Astronomico Trieste, Italy)
Bianchini, Antonio (Osservatorio Astrofisico Asiago, Italy)
Duerbeck, Hilmar W. (Muenster Univ. Germany)
Date Acquired
September 6, 2013
Publication Date
September 1, 1993
Publication Information
Publication: NASA, Washington, Cataclysmic Variables and Related Objects
Subject Category
Astronomy
Accession Number
95N27074
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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