Spectroscopic binary orbits from photoelectric radial velocities. Paper 73: HR 7041

Details Spectroscopic binary orbits from photoelectric radial velocities. Paper 73: HR 7041 Spectroscopic binary orbits from photoelectric radial velocities. Paper 73: HR 7041

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987obs...107...58g&link_type=abstract

The Observatory, vol. 107, p. 58-62 (1987)

Physics

1

Scientific paper

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.

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