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   PR #    14
   The low mass X-ray binary, 4U0614+091, that is scheduled as a
   calibrationsource, being relatively bright, steady, isolated, and not
   much absorbed,is also scheduled for ROSAT observations
   contemporaneously. On the basisof the EINSTEIN Observatory SSS
   observations, it will exhibit strongerlow energy line emission than
   the more luminous low mass X-ray binaries.Comparison of Fe K emission
   with that of the 20 times more luminousCyg X-2 would be a diagnostic
   of the location of the continuum source,the temperature, and
   ionization conditions of the inner disk and the diskcorona.
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