  Recent Chandra observations have revealed a large population of faint X-ray
point sources in the Galactic Centre. The observed population consists of about
2000 faint sources in the luminosity range ~10^31-10^33 erg/s. The majority of
these sources (70%) are described by hard spectra, while the rest are rather
soft. The nature of these sources still remains unknown. Belczynski & Taam
(2004) demonstrated that X-ray binaries with neutron star or black hole
accretors may account for most of the soft sources, but are not numerous enough
to account for the observed number and X-ray properties of the faint hard
sources. A population synthesis calculation of the Galactic Centre region has
been carried out. Our results indicate that the numbers and X-ray luminosities
of intermediate polars are consistent with the observed faint hard Galactic
Centre population.
