The microlensing objects, Machos, recently observed in the halo of our
Galaxy, can be interpreted as dense neutralino objects, neutralino st
ars, produced by the gravitational instability of neutralino gas. Taki
ng the mass and radius of these objects from microlensing observations
we calculated the diffuse gamma-ray flux produced in neutralino-neutr
alino annihilation inside the objects. The resulting flux is many orde
rs of magnitude higher than the observed one.