Photometry and analysis of the short period variability of the Nova Cygni 1975
Abstract
The UBVRI photoelectric photometry of Nova Cygni 1975 from September 1st to December 3rd is reported. Some observational features are discussed, together with some physical parameters of the binary system. An attempt to derive a theoretical model was made.
- Publication:
-
NASA STI/Recon Technical Report N
- Pub Date:
- April 1976
- Bibcode:
- 1976STIN...7634088M
- Keywords:
-
- Eclipsing Binary Stars;
- Electrophotometers;
- Novae;
- Variability;
- White Dwarf Stars;
- Brightness;
- Mathematical Models;
- Stellar Mass;
- Time Dependence;
- Astronomy