Fig. 13.
Same as Fig. 10 for NGC 613, without any black hole (left panel), with a black hole of 7.4 × 106 M⊙ (middle panel), and the best fit: 3.7 × 107 M⊙, as derived from the MBH-σ relation (Table 6) (right panel). The inclination of the torus is i = 46°. The mass model is that based on the galfit decomposition, and the predicted circular velocity is reproduced in blue lines (Fig. 9).
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