Abstract
view Abstract Citations (2) References (6) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS A possible RS Canum Venaticorum system in the Coma star cluster. Barry, D. C. Abstract 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. Publication: The Astrophysical Journal Pub Date: June 1979 DOI: 10.1086/182967 Bibcode: 1979ApJ...230L..87B Keywords: Binary Stars; Star Clusters; Stellar Spectrophotometry; Optical Emission Spectroscopy; Radio Astronomy; X Ray Astronomy; Astrophysics; Open Clusters:RS CVn Stars full text sources ADS | data products SIMBAD (3) NED (1)
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
