The eclipsing binary CW Eridani.
Abstract
Results of three-color photoelectric observations of CW Eridani are presented which were made with a 30-inch telescope over the three-year period from 1970 to 1973. The times of minima are computed, solutions of the light curves are obtained, and theoretical light curves are computed from the solutions. The period is determined to be 2.72837 days, and the orbital and photoelectric elements are derived from solutions based on the idealized Russell model.
- Publication:
-
Acta Astronomica
- Pub Date:
- 1975
- Bibcode:
- 1975AcA....25...89C
- Keywords:
-
- Eclipsing Binary Stars;
- Electrophotometry;
- Light Curve;
- Stellar Spectrophotometry;
- Tables (Data);
- Absorption Spectra;
- Data Reduction;
- Stellar Spectra;
- Ultraviolet Spectra;
- Astronomy