Spectroscopic binaries near the North Galactic Pole: Paper 15 - HD 106947

Details Spectroscopic binaries near the North Galactic Pole: Paper 15 - HD 106947 Spectroscopic binaries near the North Galactic Pole: Paper 15 - HD 106947

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988japa....9..127g&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 9, Sept. 1988, p. 127-136.

Astronomy and Astrophysics

Astrophysics

3

Angular Velocity, Astronomical Spectroscopy, Binary Stars, Star Clusters, Astronomical Models, Radial Velocity, Stellar Orbits

Scientific paper

Photoelectric radial-velocity measurements show that HD 106947 is a
double-lined spectroscopic binary. The components have spectral types of
about F6 V and G5 V and are in a 59-day orbit of moderate eccentricity.
The system is a member of the Coma Cluster.

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