The giant spectroscopic binary 35 Comae

Details The giant spectroscopic binary 35 Comae The giant spectroscopic binary 35 Comae

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100..358g&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, March 1988, p. 358-361.

Astronomy and Astrophysics

Astronomy

4

Binary Stars, Giant Stars, Late Stars, Stellar Motions, Eccentric Orbits, Orbital Elements, Radial Velocity, Star Clusters, Stellar Mass

Scientific paper

The authors show that 35 Com A (=HR 4894, HD 112033, the brightest
component of ADS 8659) is a spectroscopic binary. It has a very
eccentric orbit and a period of 8 years. There is no significance in the
anomalously large mass that has sometimes been attributed to the system.

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