Spectroscopic binary orbits from photoelectric radial velocities. Paper 73: HR 7041
Abstract
HR 7041 is a very red sixth-magnitude star, probably an M giant, near Vega. It is a spectroscopic binary with an extremely eccentric orbit and a period of 8 years. It has a tenth-magnitude visual companion, which is shown not to be physically associated with it.
- Publication:
-
The Observatory
- Pub Date:
- April 1987
- Bibcode:
- 1987Obs...107...58G