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   PR # 41155
   EGRET has found almost 30 Gamma-ray sources near the galactic plane
   (gb <+-10 deg). Among them five sources are identified as pulsars,
   such as Geminga. However, most of them have not been identified with
   any known sources. A few hundred MeV to GeV emission from galactic
   source is particulary interesting. Pulsar could be one possibility
   and galactic objects with jets directed toward the solar system could
   be another possibility. Because of the high galactic absorption, hard
   X-ray observation with ASCA is crucial to reveal the nature of the
   source. We propose to observe the brightest, thus with the smallest
   error circle, unidentified EGRET source, near Cygnus Complex.
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