Bright novae in M31 and the relationship between their maximum brightness and rate of decline

Details Bright novae in M31 and the relationship between their maximum brightness and rate of decline Bright novae in M31 and the relationship between their maximum brightness and rate of decline

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15...11s&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Jan. 1989, p. 11-16. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

4

Andromeda Galaxy, Novae, Brightness Distribution, Stellar Luminosity, Stellar Magnitude

Scientific paper

The relationship between the maximum brightness and the rate of decline
of novae in M 31 is considered. It is shown that the fastest novae are
more luminous than previously believed. Data are presented on the nova
detected in 1983.

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