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HD 115781 and HD 116204—two RS CVn binaries
DOI: 10.1007/BF02715066 Bibcode: 1988JApA....9..213G

Fekel, Francis C.; Griffin, R. F.

HD 115781 and HD 116204 (BL CVn and BM CVn) are shown to be RS CVn binaries with periods near 20 days. HD 115781 is double-lined; the primary type is about K1III, while the secondary is probably a late-type subgiant. The masses of the two components are equal within observational error. There is substantial photometric variability with a period ha…

1988 Journal of Astrophysics and Astronomy
IUE 11