******************************************************
   PR # 41050
   ASCA has opened a new window, spectroscopy of Galactic globular
   clusters. From AO2 observations of nearby King-Model (KM) clusters,
   Omega Centauri and M22, we obtained spectra of dim X-ray sources
   associated with and without the clusters for the first time. They
   allow us to identify the dim X-ray sources as CVs and normal stars.
   As a nest step, we propose observations of nearby Post-Core-Collapsed
   (PCC) clusters, NGC 6139 and NGC 6544. These observations will
   provide spectra of known and unkown X-ray sources. Together with the
   previous results, they are useful pieces of information on the
   cluster evolution from KM clusters to PCC ones.
  ******************************************************