  We present analysis of medium resolution optical spectra and long term V band
photometry of four cool stars, BD+13 5000, BD+11 3024, TYC 3557-919-1 and TYC
5163-1764-1. Our spectroscopic analysis reveals that the stars are giant or
sub-giant from K0 or K1 spectral type, and all of them exhibit emission
features in their Ca ii H& K lines. These features appear to be modulated with
the rotation of the stars. Except BD+11 3024, we observe that the radial
velocities of the target stars are not stable, which suggests that each of them
might be a member of a binary system. Global analysis of photometric data
indicates clear cyclic variation for BD+13 5000 and TYC 5163-1764-1 with a
period of 8.0$\pm$0.3 and 5.04$\pm$0.04 year, respectively. Besides that, we
observe a dramatic increase ($\sim$0\fm7) in the mean brightness of BD+11 3024,
accompanied with a 2.87$\pm$0.12 cyclic variation, embedded into the global
brightening trend, which indicates possible multiple cycles on this star.
