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V 1500 Cyg: Slow Variability in Post-nova Stage
Published online by Cambridge University Press: 12 April 2016
Extract
Regular photometric observations of V1500 Gyg (Nova Cygni 1975) have been carried out at the Crimean Astrophysical Observatory of the USSR Academy of Sciences from 1975 till now. The 0.5 m telescope equipped with a TV system is used to estimate the star brightness in V.
The decline of the mean brightness is presented in Figure 1. The solid lines (1) and (2) show the changes of the V brightness according to Patterson (1979) and Arkhipova and Zaitseva (1978), respectively. The dotted line is drawn according to our data (Pavlenko 1988). The arrows indicate the amplitudes of the light and colour variations.
- Type
- 1a. Basic Properties of Novae
- Information
- International Astronomical Union Colloquium , Volume 122: Physics of Classical Novae , 1990 , pp. 68 - 70
- Copyright
- Copyright © Springer-Verlag 1990