Do Nuclear Star Clusters and Supermassive Black Holes Follow the Same Host-Galaxy Correlations?
Table 2
Galaxies with well-determined NSC masses.
Name
(err)
Type
Source
Total (err)
Bulge (err)
(Mpc)
Milky way
4
0.01
7.48 (0.09)
D
1
10.74 (0.09)
10.00 (0.13)
M31
3
0.77
7.54 (0.06)
D
2
10.92 (0.06)
10.27 (0.11)
M33
6
0.81
6.24 (0.08)
D
3
9.74 (0.08)
8.44 (0.12)
IC342
6
3.37
7.05 (0.07)
D
4
10.23 (0.07)
8.82 (0.23)
NGC300
7
2.02
5.98 (0.06)
D
5
9.26 (0.06)
< 6.26
NGC404
−3
3.18
7.04 (0.06)
D
6
9.24 (0.06)
9.06 (0.11)
NGC428
9
15.5
6.51 (0.18)
D
5
9.81 (0.18)
7.76 (0.29)
NGC1042
6
17.5
6.51 (0.18)
D
5
10.14 (0.18)
7.98 (0.21)
NGC1493
6
11.0
6.38 (0.19)
D
5
9.75 (0.19)
< 6.75
NGC1705
−3
5.11
4.91 (0.12)
D
7
8.38 (0.12)
7.87 (0.15)
NGC2139
6
22.9
5.92 (0.18)
D
5
10.15 (0.18)
< 7.15
NGC3423
6
14.4
6.53 (0.19)
D
5
10.08 (0.19)
8.91 (0.21)
NGC3621
7
6.64
7.00 (0.08)
D
8
10.20 (0.08)
8.25 (0.14)
NGC5457
6
7.05
6.91 (0.09)
D
9
10.68 (0.09)
8.76 (0.24)
NGC6946
6
5.89
7.88 (0.10)
D
9
10.62 (0.10)
9.36 (0.13)
NGC7418
6
17.8
7.78 (0.18)
D
5
10.29 (0.18)
8.50 (0.19)
NGC7424
6
10.5
6.09 (0.18)
D
5
9.53 (0.18)
8.29 (0.19)
NGC7793
7
3.91
6.96 (0.11)
D
5
9.65 (0.11)
8.01 (0.14)
NGC1325
4
19.6
7.08 (0.18)
S
10
10.34 (0.18)
7.91 (0.20)
NGC1385
6
18.1
6.39 (0.18)
S
10
10.28 (0.18)
8.69 (0.20)
NGC2552
9
9.68
5.77 (0.18)
S
10
9.00 (0.18)
6.30 (0.28)
NGC3177
3
19.6
8.15 (0.18)
S
10
10.10 (0.18)
8.71 (0.20)
NGC3277
2
21.4
8.34 (0.18)
S
10
10.32 (0.18)
…
NGC3455
3
16.4
6.75 (0.18)
S
10
9.46 (0.18)
…
NGC4030
4
20.5
7.99 (0.18)
S
10
10.92 (0.18)
10.28 (0.20)
NGC4411B
6
18.6
6.53 (0.19)
S
10
9.46 (0.19)
…
NGC4701
6
10.8
6.53 (0.18)
S
10
9.34 (0.18)
…
NGC4775
7
21.9
7.60 (0.19)
S
10
10.19 (0.19)
8.76 (0.20)
NGC5377
1
28.4
8.63 (0.18)
S
10
10.80 (0.18)
…
NGC5585
7
8.71
5.87 (0.19)
S
10
9.26 (0.19)
8.58 (0.21)
NGC5806
3
20.0
8.11 (0.18)
S
10
10.43 (0.18)
…
NGC7421
4
23.1
6.87 (0.18)
S
10
10.24 (0.18)
…
NGC7690
3
17.7
7.98 (0.18)
S
10
9.90 (0.18)
9.28 (0.20)
(1) Galaxy name. (2) Hubble type from RC3. (3) Adopted distance in Mpc. (4) Logarithm of NSC mass and uncertainty; masses have been rescaled using the distances column 2, if necessary. Errors are 1- values. (5) Type of NSC mass measurement: D: dynamical, S: spectroscopic. (6) Source of NSC measurement: 1 = Launhardt et al. [31]; 2 = Kormendy and Bender [25]; 3 = Matthews et al. [26] + Gebhardt et al. [27]; 4 = Böker et al. [24]; 5 = Walcher et al. [21]; 6 = Seth et al. [29]; 7 = Ho and Filippenko [23]; 8 = Barth et al. [28]; 9 = Kormendy et al. [30]; 10 = Rossa et al. [11]. (7) Logarithm of total galaxy stellar mass and uncertainty (see text for details). (8) Logarithm of bulge stellar mass and uncertainty (or upper limit for bulgeless galaxies), based on decompositions in Erwin and Gadotti (2012a, in prep); galaxies currently missing proper decompositions are indicated by “…”.
