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   PR #    35
   MCG -2-58-022 is a bright AGN appearing in the HEAO-1 A2 survey.
   Thegalaxy shows strong Fe~K emission (150 eV equiv. width) and
   possibleFe~L emission (also 150 eV equiv. width). If ASCA can confirm
   thatthe soft lines are truly Fe, then the ratio of K/L flux will allow
   testingof models as to whether the central X-ray emission is
   anisotropic. Inaddition the Fe K line profile alone allows critical
   testing of accretiondisk models, and testing of photoionization models
   by the ratio of Fe Lto the continuum.
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