Spectroscopic binaries near the north galactic pole. XXII - HR 4793

Details Spectroscopic binaries near the north galactic pole. XXII - HR 4793 Spectroscopic binaries near the north galactic pole. XXII - HR 4793

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992japa...13..209g&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 13, no. 2, June 1992, p. 209-216. Research supported by SERC and NS

Astronomy and Astrophysics

Astrophysics

6

Astronomical Spectroscopy, Binary Stars, Circular Orbits, Galactic Structure, Stellar Orbits, Astronomical Photometry, Radial Velocity, Stellar Spectra

Scientific paper

Results are presented on photoelectric radial-velocity observations of a
K1 III star HR 4793, made by several observatories. The data indicate
that the HR 4793 is a spectroscopic binary. It has a circular orbit with
a period of 111 days and an amplitude of 7 km/sec.

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