  The galactic center excess is a possible non-gravitational observation of
dark matter; however, the canonical dark matter model (thermal freeze-out) is
in conflict with other gamma-ray observations, in particular those made of the
Milky Way's satellite dwarf galaxies. Here we consider the effects of a
two-component dark matter model which results in minimally boosted particles
that must remain bound to their host galaxy in order to produce an
observational signal. This leads to a signal that is heavily dependent on
galactic scale and can help reconcile the differences in the galactic center
and dwarf galaxy measurements under the dark matter paradigm.
