  We present first results of a campaign to find and identify new compact
objects in the Galactic Center. Selecting candidates from a combination of
Chandra and 2MASS survey data, we search for accretion disk signatures via
infrared spectroscopy. We have found the infrared counterpart to the Chandra
source CXO J174536.1-285638, the spectrum of which has strong Br-gamma and HeI
emission. The presence of CIII, NIII, and HeII indicate a binary system. We
suspect that the system is some form of high-mass binary system, either a
high-mass X-ray binary or a colliding wind binary.
