Bright novae in M 31 and the relation between maximum magnitude and rate of decline.
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.
Pisma v Astronomicheskii Zhurnal
- Pub Date:
- January 1989
- Andromeda Galaxy;
- Brightness Distribution;
- Stellar Luminosity;
- Stellar Magnitude;