Table 2.
Properties of nuclear discs, bars and galaxies in the TIMER sample.
Galaxy | v/σ | rk | re, K | re, S | Rbar | ϵbar | Bar/T | QB | A2 | R25.5 |
---|---|---|---|---|---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
IC 1438 | 2.57 | 0.60 | 0.77 | 0.56 | 4.43 | 0.53 | 0.11 | 0.178 | 0.838 | 12.76 |
NGC 613 | 2.35 | 0.59 | 0.71 | 0.68 | 9.72 | 0.62 | 0.26 | 0.489 | 0.903 | 23.60 |
NGC 1097 | 2.82 | 1.07 | 0.95 | 1.24 | 10.40 | 0.45 | 0.26 | 0.254 | 0.709 | 36.24 |
NGC 1300 | 2.98 | 0.33 | 0.44 | 0.38 | 6.70 | 0.75 | 0.08 | 0.58 | 0.603 | 17.88 |
NGC 1433 | 2.00 | 0.38 | 0.42 | 0.42 | 3.63 | 0.68 | 0.08 | 0.366 | 0.560 | 12.82 |
NGC 3351 | 2.57 | 0.24 | 0.41 | 0.33 | 4.02 | 0.70 | 0.09 | 0.227 | 0.513 | 12.41 |
NGC 4303 | 1.36 | 0.21 | 0.39 | 0.29 | 3.52 | 0.56 | 0.06 | 0.535 | 0.550 | 18.14 |
NGC 4371 | 2.02 | 0.95 | 0.82 | 0.234 | 0.618 | 16.38 | ||||
NGC 4643 | 1.31 | 0.50 | 0.86 | 0.272 | 0.813 | 24.45 | ||||
NGC 4981 | 0.99 | 0.14 | 0.29 | 0.093 | 0.172 | 13.56 | ||||
NGC 4984 | 2.49 | 0.49 | 0.53 | 0.55 | 6.18 | 0.48 | 0.14 | 0.176 | 0.836 | 18.98 |
NGC 5236 | 1.89 | 0.37 | 0.32 | 0.472 | 0.467 | 19.35 | ||||
NGC 5248 | 1.66 | 0.49 | 0.58 | 0.138 | 0.324 | 17.28 | ||||
NGC 5728 | 2.84 | 0.63 | 0.83 | 0.86 | 9.70 | 0.51 | 0.28 | 0.387 | 1.149 | 20.58 |
NGC 5850 | 1.13 | 0.80 | 0.62 | 0.74 | 7.84 | 0.64 | 0.16 | 0.327 | 0.742 | 20.80 |
NGC 7140 | 1.45 | 0.63 | 0.99 | 0.66 | 11.16 | 0.36 | 0.23 | 0.399 | 0.805 | 24.86 |
NGC 7552 | 2.61 | 0.33 | 0.34 | 0.36 | 4.90 | 0.64 | 0.32 | 0.358 | 1.060 | 9.79 |
NGC 7755 | 2.20 | 0.47 | 0.53 | 0.401 | 0.841 | 20.29 |
Notes. Column (1) gives the galaxy designation, while Cols. (2) and (3) show, respectively, the peak value of v/σ in the nuclear disc, and the radius at which this peak is located, rk. In Cols. (4) and (5) we show the effective radius of the photometric bulge derived by Kim et al. (2014) and Salo et al. (2015), respectively. Columns (6)−(8) present the bar radius, ellipticity and bar-to-total luminosity ratio as derived by Kim et al. (2014). In Cols. (9) and (10) we present the values of QB and A2 calculated by Díaz-García et al. (2016). Finally, Col. (11) shows the values of R25.5 obtained by Muñoz-Mateos et al. (2015). All radii are in kpc, using the distances tabulated in Paper I, and the bar radii and ellipticities derived by Kim et al. are deprojected following the 2D approach described in Gadotti et al. (2007).
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