  A dissipative dark sector can result in the formation of compact objects with
masses comparable to stars and planets. In this work, we investigate the
formation of such compact objects from a subdominant inelastic dark matter
model, and study the resulting distributions of these objects. In particular,
we consider cooling from dark Bremsstrahlung and a rapid decay process that
occurs after inelastic upscattering. Inelastic transitions introduce an
additional radiative processes which can impact the formation of compact
objects via multiple cooling channels. We find that having multiple cooling
processes changes the mass and abundance of compact objects formed, as compared
to a scenario with only one cooling channel. The resulting distribution of
these astrophysical compact objects and their properties can be used to further
constrain and differentiate between dark sectors.
