Table 2
Luminosities and other properties for the whole LLAGN sample.
Object | AGN type | D | Ref. | r0 | log NH | log L2−10 keV | log λL12 μm | log MBH | Ref. | log λEdd |
[Mpc] | [pc] | cm-2 | [erg/s] | [erg/s] | [M⊙] | |||||
|
||||||||||
NGC 676 | Sy 2.0 | 19.5 ± 8.7 | 18 | 33 | >24.3 | 40.79 ± 0.60 | <40.84 | 7.56 | 10 | <–4.0 |
NGC 1052 | L | 18.0 ± 2.4 | 12 | 31 | 23.1 | 41.18 ± 0.30 | 42.13 ± 0.07 | 8.19 | 10 | –3.8 |
NGC 1097 | L | 19.1 ± 4.2 | 19 | 32 | 20.4 | 40.88 ± 0.15 | 41.23 ± 0.06 | 8.08 | 13 | –4.2 |
NGC 1386 | Sy 2.0 | 18.3 ± 1.4 | 14 | 31 | > 24.3 | 42.10 ± 0.60 | 42.26 ± 0.01 | 7.78 | 11 | –2.9 |
NGC 1404 | 16LG | 18.3 ± 1.4 | 14 | 31 | <22.0 | 39.92 ± 0.30 | <41.25 | 8.50 | 11 | <–5.2 |
NGC 1566 | Sy 1.5 | 14.3 ± 5.9 | 1 | 24 | <22.0 | 41.62 ± 0.30 | 41.76 ± 0.06 | 7.01 | 11 | –2.6 |
NGC 1667 | Sy 2.0 | 62.6 ± 4.3 | 16 | 106 | > 24.3 | 42.33 ± 0.60 | <42.25 | 7.81 | 11 | <–2.8 |
ESO 005-G004 | Sy 2.0 | 22.4 ± 10.0 | 18 | 38 | 24.0 | 41.82 ± 0.30 | 42.00 ± 0.08 | 7.89 | 20 | –3.2 |
NGC 3125 | L | 19.8 ± 1.4 | 16 | 34 | 21.7 | 40.14 ± 0.30 | 41.87 ± 0.08 | 5.77 | 5 | –2.0 |
NGC 3312 | L | 44.7 ± 3.1 | 16 | 76 | <22.0 | 41.10 ± 0.60 | <42.15 | 8.28 | 11 | <–3.9 |
NGC 4235 | Sy 1.2 | 35.2 ± 15.7 | 18 | 60 | 21.2 | 41.61 ± 0.30 | 42.08 ± 0.05 | 7.60 | 10 | –3.0 |
NGC 4261 | L | 29.4 ± 2.7 | 12 | 50 | 23.2 | 41.00 ± 0.30 | 41.58 ± 0.05 | 8.72 | 6 | –4.7 |
NGC 4303 (M 61) | Sy 2.0 | 15.2 ± 3.1 | 18 | 26 | <22.0 | 39.04 ± 0.30 | 40.72 ± 0.23 | 6.52 | 10 | –3.9 |
NGC 4472 (M 49) | Sy 2.0 | 17.1 ± 0.6 | 15 | 29 | <22.0 | 39.00 ± 0.30 | <41.05 | 8.81 | 10 | <–6.0 |
NGC 4486 (M 87) | L | 17.1 ± 0.6 | 15 | 29 | 22.6 | 40.73 ± 0.30 | 41.26 ± 0.05 | 9.82 | 9 | –6.1 |
NGC 4579 (M 58) | L | 16.8 ± 3.4 | 18 | 29 | 21.7 | 41.18 ± 0.15 | 41.70 ± 0.06 | 7.77 | 10 | –3.6 |
NGC 4594 (M 104) | Sy 1.9 | 9.1 ± 0.8 | 12 | 15 | 21.3 | 39.99 ± 0.30 | <40.61 | 8.46 | 10 | <–5.4 |
NGC 4698 | Sy 2.0 | 23.8 ± 6.4 | 17 | 40 | > 24.3 | 40.82 ± 0.60 | <41.30 | 7.57 | 10 | <–3.8 |
NGC 4941 | Sy 2.0 | 19.8 ± 1.4 | 16 | 34 | 23.7 | 41.43 ± 0.30 | 41.94 ± 0.02 | 6.91 | 11 | –2.5 |
NGC 5128 (Cen A) | Sy 2.0 | 3.4 ± 0.2 | 7 | 6 | 23.0 | 41.69 ± 0.15 | 41.71 ± 0.01 | 7.74 | 4 | –3.3 |
NGC 5363 | L | 19.4 ± 1.4 | 16 | 33 | > 24.3 | 41.44 ± 0.60 | <41.30 | 8.36 | 10 | <–4.2 |
NGC 5813 | L | 32.1 ± 2.8 | 2 | 54 | 21.1 | 38.77 ± 0.30 | <42.19 | 8.53 | 10 | <–5.3 |
NGC 7213 | L | 21.2 ± 1.5 | 16 | 36 | 20.3 | 42.09 ± 0.15 | 42.48 ± 0.03 | 7.74 | 11 | –2.7 |
IC 1459 | Sy 2.0 | 30.3 ± 4.2 | 2 | 51 | 22.1 | 40.61 ± 0.30 | <41.91 | 9.41 | 3 | <–5.4 |
NGC 7590 | Sy 2.0 | 27.4 ± 6.0 | 19 | 47 | <22.0 | 39.77 ± 0.60 | <41.79 | 6.71 | 8 | <–3.2 |
NGC 7626 | L | 41.9 ± 2.9 | 16 | 71 | <22.0 | 39.56 ± 0.30 | <42.13 | 8.78 | 10 | <–5.2 |
NGC 7743 | Sy 2.0 | 19.2 ± 1.6 | 12 | 33 | > 24.3 | 41.27 ± 0.60 | <41.15 | 6.64 | 10 | <–2.7 |
Notes. References on distances and black hole masses. (1) average of Tully (1988), Willick et al. (1997) and DL from NED; (2) Blakeslee et al. (2001); (3) Cappellari et al. (2002); (4) Cappellari et al. (2009); (5) Dudik et al. (2005); (6) Ferrarese et al. (1996); (7) Ferrarese et al. (2007); (8) Garcia-Rissmann et al. (2005); (9) Gebhardt et al. (2011); (10) Ho et al. (2009); (11) Hyperleda database (Paturel et al. 2003); (12) Jensen et al. (2003); (13) Lewis & Eracleous (2006); (14) Madore et al. (1999); (15) Mei et al. (2007); (16) DL from NED; (17) Springob et al. (2007); (18) Tully (1988); (19) Willick et al. (1997); (29) Winter et al. (2010). r0: spatial scale corresponding to the theoretical diffraction limit for a 8.2 m VLT telescope at 12 μm. log λ = log (LBol/LEdd) is the Eddington ratio.
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.