Fig. 25
Comparison of the surface brightness of the stars (black) taken from Kormendy & Bender (1999) with ellipse fits to the fluxes of the first [O III] component (red) and the second [O III] component (magenta).The left y-axis is valid for the stellar surface brightness, the one on the right for the fluxes of the two gas components. The scales have been adjusted sothat the profiles for the stars and the first [O III] component can be compared easily.
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