A possible RS Canum Venaticorum system in the Coma star cluster

Details A possible RS Canum Venaticorum system in the Coma star cluster A possible RS Canum Venaticorum system in the Coma star cluster

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...230l..87b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 230, June 1, 1979, p. L87, L88.

Astronomy and Astrophysics

Astronomy

2

Binary Stars, Star Clusters, Stellar Spectrophotometry, Optical Emission Spectroscopy, Radio Astronomy, X Ray Astronomy

Scientific paper

The double-lined spectroscopic binary T111 (HD 108102) in the Coma
cluster of stars has many of the characteristics of RS Canum Venaticorum
systems. It is the only RS Canum Venaticorum-type system known to be a
member of a star cluster. Further observations at X-ray, optical and
radio wavelengths are suggested.

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