Fig. 7
Radial distribution of log ([O iii]/Hβ) (for active galaxies of run1) and log ([Ne iii]/Hβ) (for run2 galaxies with [Ne iii]λ3869 line detected). The theoretical curves of Kewley et al. (2001, for log ([O iii]/Hβ) and log ([N ii]/Hα)) and Rola et al. (1997, for log ([Ne iii]/Hβ)) distinguishing between AGN and SF are also plotted with dashed and solid lines, respectively.
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