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   PR #   157
   Abell 2319 is at z=.0564. Total flux is 12.1E-11, kT= 9.3 kev, Ginga
   Fe flux is1.3 ct/sec. Source is large and a offset pointing may be
   necessary for the SIS.No rosat image is available yet, but IPC image
   extends to R>17'. Weak coolingflow, M(dot)~65M/yr, no emission line
   filaments. Cooling flow not confirmedby Einstein SSS. High flux
   source, look for Fe gradient, searchfor cooling flow spectrally, good
   for SIS CTE measurement.
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