  We explore the possibility that neutron stars accreting from the winds of
main-sequence stellar companions account for a significant fraction of
low-luminosity, hard X-ray sources (L_X <~ 10^35 ergs/s; 1-10 keV) in the
Galaxy. This work was motivated by recent Chandra observations of the Galactic
center by Wang et al. (2002). Our calculations indicate that many of the
discrete X-ray sources detected in this survey may be wind-accreting neutron
stars, and that many more may be discovered with deeper X-ray observations. We
propose that an infrared observing campaign be undertaken to search for the
stellar counterparts of these X-ray sources.
