  Our star-count analysis of the Two Micron All Sky Survey point sources
resulted in an identification of the star cluster G144.9+0.4. The cluster was
found, but not characterized, by Glushkova et al. We show that the cluster is
physically associated with the Cam OB1 association at a distance of about 1 kpc
and with an age of 1-2 Myr. Pre-main sequence stars are identified on the basis
of photometric and proper motion data. A total of 91 additional OB star
candidates was found in subgroups 1A and 1B, a significant increase from the
currently known 43 OB stars. The OB members show an age spread that indicates a
sustained star formation for at least the last 10-15 Myr. The young cluster
G144.9+0.4 represents the latest episode of sequential star formation in this
cloud complex.
