Fig. 16.

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Bulge Sérsic index (n) plotted against nuclear emission type and bulge stellar mass. Core-Sérsic galaxies (enclosed in boxes) are massive and they harbor either a LINER or an ALG nucleus. The only core-Sérsic galaxy with nuclear emission associated with star-formation (H II) is the massive (M*, bulge ∼ 3.2 × 1012 M⊙) S0 NGC 3665. The blue curve connects the median Sérsic indices for the four optical emission-line classes.
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