  It has been shown that the gamma-ray flux observed by HESS from the J1745-290
Galactic Center source is well fitted as the secondary gamma-rays photons
generated from Dark Matter annihilating into Standard Model particles in
combination with a simple power law background. The neutrino flux expected from
such Dark Matter source has been also analyzed. The main results of such
analyses for 50 TeV Dark Matter annihilating into W+W- gauge boson and
preliminary results for antiprotons are presented.
