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   PR # 41132
   We propose to observe the BL Lac object PKS 0735+178, aiming to study
   physical state in its cosmical jet. This object is well observed in
   many wavelengths including GeV bands with the EGRET instrument
   onboard CGRO. Since ASCA bands would cover the connective region
   between synchrotron and its self-Comptonized components, it is
   expected to determine the ratio of two components. In addition, short
   time variability was also reported by Madejski with Einstein, which
   suggests the possibility to detect synchrotron soft-lagged variation
   to determine its magnetic field. Therefore, the source is expected to
   study magnetic field, electron density and doppler factor of the jet.
   Reported superluimnal motion will also be helpful to determine
   inclination and speed of the jet.
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