Open Access

Table 1.

Galaxy properties.

ID MBH σ vnorm Mbulge Mbulge fg Mbulge fg
(106M) (km s−1) (km s−1) (109M) (109M) (%) (109M) (%)
(from M25) (from M25) (< 1 kpc) from S19 (fit value) (fit value) (flatter fit) (flatter fit)
NGC 7582 55 140 595 14.0 16 9.3
IC 5063 174 175 2040 35.3 42 0.52
Circinus 3.5 80 491* 1.5 1.2 3.4
Centaurus A 59 140 546* 14.8 2.5 12
NGC 4945 1.4 100 1060* 0.729 2.1 0.089
IC 1657 47 143 765 12.3 27 3.7
NGC 1365 20 114 482 6.17 6.8 9.3 5.5 14
NGC 2992 23 130 705 6.9 6.8 2.8 12 14
NGC 5643 2.8 80 670* 1.25 1.4 1.1 1.5 2.5
NGC 5728 34 125 690 9.46 6.6 4.8 9.0 21

Notes. Columns show, from left to right, the galaxy ID, black hole mass (from Table 1 of M25), bulge velocity dispersion (Supplementary Fig. 3 of M25 and Cosimo Marconcini, private communication), mean outflow velocity within the central region used to normalise the velocity profile (Cosimo Marconcini, private communication), bulge mass derived from MBH using the relation in Schutte et al. (2019), bulge mass selected to produce the best fit to the outflow velocity profile, and gas fraction fg selected in the same way. For the last four galaxies, the final two columns show the bulge mass and gas fraction required when fitting a flatter bulge gas density profile. * In these galaxies, the outflow begins to accelerate within the central kiloparsec, so we recalculated the mean velocity including only the points interior to the acceleration region.

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