Beta Canum Venaticorum

Komponen dari bintang ini adalah U=−25, V=0 dan W=+2 km/s. In the past it was suggested that this star may be a
spectroscopic binary. However, further analysis of
the data does not seem to bear that out. In addition, a search for a brown dwarf in orbit around this star failed to discover any such companion, at least down to the sensitivity limit of the instrument used.