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   PR # 41146
   3C279 is a typical OVV quasar with high variability in radio through
   GeV-gamma-ray, and the brightest GeV-gamma-ray AGN. The property in
   radio to X-rays will strongly support the SSC model. However, bright
   GeV-gamma-ray flux by CGRO cannot be simply explained by this model.
   The research of GeV-gamma-ray emission mechanism unknown is expected
   to lead the origin of blazar activity, like as jets and relativistic
   electron production. We would propose the ASCA monitoring observation
   of 3C279 simultaneously with CGRO/EGRET, ROSAT, IUE and the other
   multifrequency observatries, which is the final chance of EGRET
   observation. We expect to obtain the fine correlation between the
   brightness in GeV-gamma-rays and X-rays, which is a key of the
   research of the GeV-gamma-ray emission.
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