*************************************************************************
   51016
   During the Galactic Ridge Observation program of ASCA on Mar/1996, the
   existence of a bright extended X-ray halo was observed around young
   open cluster, NGC6383. The X-ray spectrum of diffuse component show
   quite high temperature above 4keV. Such a high temperature gas cannot
   be made by stellar wind of cluster members (OB stars). To search for
   the origin of this halo(temperature and abundances), we propose 40ks
   observation to get better statistics (4 times longer exposure).
 *************************************************************************