The discovery of highly relativistic jets and superluminal motion from some x-ray binaries(Microquasars)and the tentative identification of two unidentified EGRET sources with the Microquasars LS 5030 and LSI+61 303,has revitalized the interest in these sources as candidate targets foreground based gamma-ray astronomy.Here we present a possible strategy for the MAGIC telescope to search for VHE gamma-rays from these sources,and discuss prospects off detecting hypothetical Microblazars.
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