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   71051
   Our knowledge of the Galactic X-ray sources is quite incomplete due to
   the Galactic absorption (low energy band) and limited spatial
   resolution (high energy band). Due to the limited information, we are
   till unable to answer the origin of the Galactic diffuse hot plasma,
   and characteristics of supernova remnants, X-ray pulsars, and other low
   luminosity X-ray sources. ASCA Galactic Plane and Galactic Center
   Region Survey Project that we propose is planned to cover all the
   Galactic inner disk with successive pointing observations of about 10
   ksec exposure in 50' in diameter region each. This project provides us
   with the first opportunity to remove the galactic absorption and make
   unbiased sample of many categories of the galactic X-ray sources.
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