  The extragalactic analogs of the microquasars, the quasars, are strong
gamma-ray emitters at GeV energies. It is expected that microquasars are also
gamma-ray sources, because of the analogy with quasars and because theoretical
models predict the high-energy emission. There are two microquasars that appear
as the possible counterparts for two unidentified high-energy gamma-ray
sources.
