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- W4205868051 abstract "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." @default.
- W4205868051 created "2022-01-26" @default.
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- W4205868051 date "1990-01-01" @default.
- W4205868051 modified "2023-09-27" @default.
- W4205868051 title "V 1500 Cyg: Slow Variability in Post-nova Stage" @default.
- W4205868051 cites W1964706056 @default.
- W4205868051 doi "https://doi.org/10.1017/s0252921100068391" @default.
- W4205868051 hasPublicationYear "1990" @default.
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