Spectroscopic binary orbits from photoelectric radial velocities. Paper 62: EZ Pegasi
Abstract
EZ Peg, which has had a confused history in the astronomical literature, is shown to be a double-lined spectroscopic binary with slightly unequal components (both late-G dwarfs) in a circular orbit of period 11.66 days.
- Publication:
-
The Observatory
- Pub Date:
- June 1985
- Bibcode:
- 1985Obs...105...81G