  Sub-GeV neutrinos produced in a stellar core may emerge from main sequence
stars, white dwarfs and brown dwarfs producing possible observable signals of
dark matter capture. A distribution of these stars near the Milky Way galactic
center will produce a neutrino flux that can be probed at Earth based neutrino
observatories like Super-Kamiokande. We demonstrate that this can provide a
handle to probe dark matter masses in the 100 MeV - 2 GeV mass scales that
compares favourably with present day direct detection bounds.
