Spectroscopic binary orbits from photoelectric radial velocities. Paper 72: 1 Pegasi B

Details Spectroscopic binary orbits from photoelectric radial velocities. Paper 72: 1 Pegasi B Spectroscopic binary orbits from photoelectric radial velocities. Paper 72: 1 Pegasi B

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987obs...107....1g&link_type=abstract

The Observatory, vol. 107, p. 1-5 (1987)

Computer Science

Scientific paper

The ninth-magnitude common-proper-motion companion of 1 Peg is a
single-lined spectroscopic binary whose γ-velocity is similar to
the radial velocity of the primary star in the visual system.

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