  We study the disk and accretion properties of young stars in the NGC 2068 and
NGC 2071 clusters. Using low-resolution optical spectra, we define a membership
sample and determine an age for the region of ~2 Myr. Using high-resolution
spectra of the H-alpha line we study the accretion activity of these likely
members and also examine the disk properties of the likely members using IRAC
and MIPS mid-infrared photometry. A substantial fraction (79%) of the 67
members have an infrared excess while all of the stars with significant
infrared excess show evidence for active accretion. We find three populations
of evolved disks (IRAC-weak, MIPS-weak and transition disks) all of which show
decreased accretion activity in addition to the evidence for evolution in the
dust disk.
