Table 6.
Central velocity dispersions and derived BH masses.
| Galaxy | σv | Ref. | MBH | BH/bul | SoI1 | SoI2 |
|---|---|---|---|---|---|---|
| (km s−1) | log M⊙ | % | pc | pc | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
| N613 | 122±18 | (1) | 7.57±.27 | 0.63 | 50 | 11. |
| N1326 | 111±14 | (1) | 7.40±.22 | 0.39 | 29 | 8.8 |
| N1365 | 141±19 | (1) | 7.84±.26 | 0.30 | 33 | 15. |
| N1433 | 113±3 | (2) | 7.40±.03 | 1.25 | 36 | 8.8 |
| N1566 | 98±7 | (1) | 7.13±.10 | 0.37 | 25 | 6.2 |
| N1672 | 111±3 | (2) | 7.40±.03 | 0.46 | 33 | 8.8 |
| N1808 | 138±9 | (1) | 7.79±.13 | 0.76 | 36 | 14. |
| N1068 | 174±9 | (1) | 8.23±.13 | 0.71 | 50 | 25. |
Notes. The references for the central velocity dispersion in the second column are: (1) Hyperleda compilation (http://leda.univ-lyon1.fr/). (2) Garcia-Rissmann et al. (2005) (cross-correlation method, CCM). The SoI is the radius of the sphere of influence of the black hole, the value in Col. 6 is from Merritt’s definition, M*(r < SoI1) = 2 MBH, the value in Col. 7 is SoI2 = 
.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.