Typical examples of classical novae

Details Typical examples of classical novae Typical examples of classical novae

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993nassp.507..413h&link_type=abstract

In NASA, Washington, Cataclysmic Variables and Related Objects p 413-510 (SEE N95-27068 09-89)

Astronomy and Astrophysics

Astronomy

1

Cataclysmic Variables, Infrared Astronomy, Novae, Periodic Variations, Stellar Mass Ejection, Stellar Oscillations, Stellar Spectra, Ultraviolet Astronomy, Bursts, Cygnus Constellation, Light Curve, Line Spectra, Radio Spectra, Stellar Envelopes, Stellar Mass, Visual Observation

Scientific paper

Because 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.

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