Variable stars in Local Group galaxies. VIII. A new look into the dSph galaxy Canes Venatici I
Canes Venatici I (CVnI) is a distant dwarf spheroidal galaxy (dSph) satellite of the Milky Way (MW). Recent estimates of its size and luminosity suggest that it does not belong to the ultra-faint class, but rather is similar to the classical MW dSph satellites. The aim of this work is to explore the variable stars of C...