Abundances for galaxies in our sample as determined by ASCA as a function of ﹩\mathrm{log}\,\,( L^{h}_{\mathrm{X}\,}/L_{B}) ﹩ with 90% error bars. Open triangles denote values from Matsumoto et al. (1997), open squares denote values from Loewenstein (1996), filled triangles denote values from Buote & Canizares (1997), and filled squares denote values from Arimoto et al. (1997).