  I present preliminary BV resolved stellar photometry of the M31 disk measured
from the data set of the NOAO/CTIO Local Group Survey. I have performed
detailed analyses of the star formation histories in and around three currently
active regions in the M31 disk: OB 78, OB 102 and the northeast spiral arm. The
results suggest that low H$\alpha$ emission from OB 78 compared to other active
regions is directly related to the details of the recent star formation
histories of the regions. In addition, while every active region I analyzed
shows a recent increase in star formation activity, some active regions also
contain overdensities of stars with ages <~100 Myr compared to adjacent
regions. The adjacent regions show a relatively constant, low star formation
rate over the past 100 Myr. There is no significant difference between the
stellar populations on either side of the active regions. This symmetry
provides no obvious signature of recent propagation of star formation near
these currently active regions of the M31 disk.
