  Nine new short period variable stars have been discovered in the direction of
the open cluster Cr464 in Camelopardalis. The field was observed using Tzec
Maun Observatory's telescope AP180. Two new variable stars were classified as
pulsating stars (RRab and RRc types). The other seven stars are binary systems.
One of them is of ELL-type, four binaries were recognized as EW-type, and two
systems are rather short period EA-type binaries. All new variables were
registered in the VSX catalogue.
