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    PR # 31138                                                                   
     The X-ray emissions from X-ray faint early-type galaxies can be fit e       
     qually  well (i) by a two-temperature solar abundance model with a Ve       
     ry Soft Component  (VSC) and a hard component (ii) by a one-temperatu       
     re model with near zero  abundance. A 60 ksec pointing of the standar       
     d elliptical galaxy NGC 3379 can  clearly establish or rule out the i       
     mportance of the VSC in a normal elliptical  galaxy. The SB0 galaxy N       
     GC 3384 is in the same ASCA field of view so the VSC  hypothesis can        
     be tested independently on two early-type galaxies  simultaneously. D       
     ue to NGC 3379s proximity we will get the highest spectral  and spati       
     al resolution of an archetypical elliptical galaxy attainable with  A       
     SCA; giving clues to X-ray emission mechanisms in early-type galaxies       
     in  general: Stellar and/or g                                               
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