Table 5.
Rotation curves and mass models for three lenticular galaxies.
Galaxy | R [kpc] | vobs [km s−1] | ev, obs [km s−1] | vH2 [km s−1] | vHI [km s−1] | vdisk [km s−1] | vbulge [km s−1] | ΣH2 [L⊙ pc−2] | ΣHI [L⊙ pc−2] | Σdisk [L⊙ pc−2] | Σbulge [L⊙ pc−2] |
---|---|---|---|---|---|---|---|---|---|---|---|
0.38 | 140 | 29 | 17.82 | 0.95 | 222.95 | − | 120.89 | 2.61 | 8422.37 | − | |
1.15 | 194 | 29 | 39.08 | 2.83 | 243.31 | − | 60.77 | 2.54 | 1238.20 | − | |
1.92 | 211 | 29 | 44.22 | 4.48 | 234.68 | − | 18.87 | 2.46 | 506.32 | − | |
NGC 2824 | 2.88 | 160 | 10 | 38.55 | 6.39 | 209.06 | − | 3.96 | 2.37 | 139.56 | − |
4.81 | 160 | 11 | 28.95 | 10.31 | 169.19 | − | 0.19 | 2.25 | 59.68 | − | |
6.73 | 160 | 8 | 23.76 | 14.80 | 151.28 | − | 0.01 | 1.90 | 17.84 | − | |
8.65 | 160 | 10 | 20.70 | 17.82 | 132.94 | − | 0.00 | 1.28 | 10.12 | − | |
0.22 | 147 | 15 | 7.48 | −0.22 | 199.14 | − | 63.93 | 2.04 | 23094.69 | − | |
0.67 | 182 | 15 | 19.16 | 1.75 | 265.53 | − | 49.70 | 1.97 | 3566.60 | − | |
1.11 | 214 | 15 | 28.68 | 2.78 | 258.78 | − | 34.04 | 1.90 | 1747.42 | − | |
1.55 | 220 | 30 | 32.82 | 3.70 | 251.56 | − | 13.32 | 1.82 | 1233.41 | − | |
2.00 | 237 | 30 | 29.53 | 4.55 | 254.81 | − | 0.74 | 1.75 | 1048.37 | − | |
4.99 | 197 | 15 | 16.26 | 8.79 | 239.53 | − | 0 | 1.26 | 157.55 | − | |
NGC 3626 | 8.32 | 157 | 12 | 9.44 | 10.36 | 199.06 | − | 0 | 0.87 | 36.76 | − |
11.65 | 158 | 11 | 10.50 | 11.29 | 173.70 | − | 0 | 0.92 | 13.83 | − | |
14.98 | 169 | 7 | 9.25 | 15.36 | 154.07 | − | 0 | 0.92 | 3.18 | − | |
18.31 | 180 | 9 | 8.37 | 20.41 | 138.64 | − | 0 | 0.49 | 0 | − | |
21.64 | 191 | 12 | 7.70 | 18.97 | 124.74 | − | 0 | 0.21 | 0 | − | |
24.97 | 198 | 11 | 7.15 | 17.64 | 115.31 | − | 0 | 0.09 | 0 | − | |
0.38 | 120 | 14 | 30.50 | 0.74 | 20.39 | 125.74 | 229.04 | 1.83 | 390.16 | 2782.91 | |
UGC 06176 | 3.81 | 137 | 8 | 27.18 | 6.53 | 87.10 | 154.91 | 0.06 | 1.55 | 175.01 | 0.04 |
11.43 | 137 | 8 | 15.15 | 14.76 | 56.18 | 50.28 | 0 | 0.87 | 1.92 | 0 | |
19.05 | 137 | 8 | 11.77 | 17.81 | 41.33 | 38.95 | 0 | 0.29 | 0 | 0 |
Notes. Sampled radii (R), observed rotation velocities (vobs), and relative errors (ev, obs) from CO and HI datacubes. Contributions to the circular velocity from the molecular gas disk (vH2), atomic gas disk (vHI), stellar disk (vd), and -if present- stellar bulge (vb), together with the corresponding surface densities at R. For convenience, the velocity contributions and surface density profiles of the stellar disk and the bulge are normalized to a mass-to-light ratio of 1 at 3.6 μm.
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