Status : Chromospherically active binary stars whose components are on the main sequence. X-ray emission is possible.
Spectral type : G-K-M and luminosity type V.
Variability : Rotating variable stars with periods from about 1 to 120 days and amplitudes smaller than 0.5 mag in V. Some of them are also Flare stars similar to UV Cet variables. Corresponding type in the GCVS : BY (eventually + UV).
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CecileLoup - 2014-04-08
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AdaNebot - 2014-11-27