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    PR # 32153                                                                   
     We propose to observe the compact elliptical galaxy NGC 4291 with           
     ASCA for 40 ksec in order to measure the metallicity of its hot             
     interstellar gas. ASCA PV phase observations of elliptical galaxies         
     suggest a relationship between compactness at optical and X-ray             
     wavelengths and metallicity that may reveal a fundamental connection        
     between baryon-to-nonbaryon ratio, dissipation in galaxy formation,         
     and metal enrichment. NGC 4291 is the only suitable galaxy bright           
     enough to test this connection. We will also obtain GIS and SIS             
     spectra of MKN 205 that can be used to study the flux and spectral          
     variability of this quasar.                                                 
                                                                                 
                                                                                 
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