  We study the indirect detection of dark matter when the local dark matter
velocity distribution depends upon position, as expected for the Milky Way and
its dwarf spheroidal satellites, and the annihilation cross-section is not
purely s-wave. Using a phase-space distribution consistent with the dark matter
density profile, we present estimates of cosmic and gamma-ray fluxes from dark
matter annihilations. The expectations for the indirect detection of dark
matter can differ significantly from the usual calculation that assumes that
the velocity of the dark matter particles follows a Maxwell-Boltzmann
distribution.
