  The stellar content of the debris field around M81 is investigated using deep
images obtained with MegaCam on the Canada-France-Hawaii Telescope. Three new
concentrations of bright main sequence stars and red supergiants are identified
within ~ 20 kpc of M81. These systems have integrated brightnesses M_V ~ -11
and surface brightnesses ~ 27 - 28 mag per arcsec^2 in V. The main sequence
turn-offs are consistent with an age of ~ 30 Myr, while the presence of a
well-developed red supergiant plume indicates that their stellar content is not
coeval, as they also formed stars ~ 100 Myr in the past. The photometric
properties of the red supergiants indicate that the young stars in these
systems have metallicities that are comparable to those of other objects in the
debris field. The HI density near these groupings comfortably exceeds the
threshold required to trigger star formation. Based on the close proximity of
these objects to M81, coupled with their extended sizes and low inferred
masses, it is argued that they will not be long-lived structures, but will
probably dissipate within the next ~ 1 Gyr.
