*************************************************************************
   61080
   We have observed the Galactic Center region with ASCA, and got many
   fruitful results. The region around (l,b)=(359,-1) is the special
   region where many high-energy phenomena are known, but not observed
   with ASCA. In this region, there are peculiar radio non-thermal
   structure "the Mouse", two X-ray bursters SLX 1744-299/300, and shell-
   type SNR G359.0-0.9. Our goal is solving each physics of them on the
   viewpoint of high energy phenomena, and then finding the phenomena or
   laws which can be applied to the whole Galactic Center region.
   Especially, our first objective is detecting the hard X-ray emission
   corresponding to the Mouse, solving the emission mechanism and its
   origin.
 *************************************************************************