Spectroscopic orbit of the star HR 96.
Abstract
The rather long orbital period of 48.2905 days and large eccentricity of 0.384, together with a mass function of 0.107, are derived for the spectroscopic binary HR 96. The extensive photographic plate material employed in the present study does not support previously suggested spectroscopic and photometric peculiarities and variability.
- Publication:
-
Astronomy and Astrophysics Supplement Series
- Pub Date:
- July 1983
- Bibcode:
- 1983A&AS...53...29H
- Keywords:
-
- Astrometry;
- B Stars;
- Binary Stars;
- Orbital Elements;
- Eclipsing Binary Stars;
- Radial Velocity;
- Astronomy