Table 5
Parameterization of the orientation and kinematics of the galaxy disks.
UGC | V sys | φ 0 | κ K | M K |
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i TF |
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(km s-1) | (deg) | (mag) | (mag) | (km s-1) | (km s-1) | (deg) | (km s-1) | (arcsec) | (km s-1) | (arcsec) | |
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
|
|||||||||||
448 | 4856.8 ± 0.5 | 306.1 ± 0.6 | −0.04 | −23.93 ± 0.10 | 186 ± 11 | 83.3 ± 0.6 | 26.6 ± 1.6 | 79.0 ± 0.8 | 5.06 ± 0.45 | 82.1 ±1.0 | 4.55 ±0.62 |
463 | 4459.4 ± 0.6 | 68.5 ± 0.6 | −0.04 | −24.49 ± 0.09 | 209 ± 12 | 106.2 ± 0.5 | 30.6 ± 1.9 | 99.7 ± 0.7 | 10.79 ± 0.33 | 107.5 ±1.3 | 9.67 ±0.53 |
1081 | 3135.2 ± 0.4 | 72.5 ± 0.6 | −0.03 | −23.05 ± 0.14 | 156 ±9 | 62.7 ± 1.4 | 23.8 ± 1.6 | 58.7 ± 1.0 | 13.74 ± 0.80 | 63.8 ±1.9 | 15.59 ±1.69 |
1087 | 4480.9 ± 0.6 | 84.8 ± 1.0 | −0.04 | −23.18 ± 0.13 | 160 ± 10 | 59.6 ± 0.5 | 21.9 ± 1.4 | 50.4 ± 1.6 | 7.07 ± 0.80 | 58.6 ±1.0 | 5.09 ±0.95 |
1529 | 4648.5 ± 0.7 | 162.1 ± 0.9 | −0.04 | −23.96 ± 0.11 | 187 ± 11 | 118.8 ± 0.5 | 39.4 ± 2.6 | 118.4 ± 1.1 | 7.91 ± 0.40 | 121.1 ±1.6 | 7.01 ±0.58 |
1635 | 3516.5 ± 0.5 | 145.0 ± 1.0 | −0.03 | −22.93 ± 0.13 | 152 ±9 | 53.4 ± 0.5 | 20.6 ± 1.3 | 50.5 ± 1.0 | 9.41 ± 0.71 | 53.7 ±1.5 | 11.04 ±1.30 |
1862 | 1388.1 ± 0.5 | 20.6 ± 1.4 | −0.01 | −20.96 ± 0.27 | 102 ±8 | 57.1 ± 2.0 | 34.2 ± 3.3 | 46.6 ± 1.6 | 17.95 ± 1.51 | 56.6 ±3.2 | 18.89 ±2.33 |
1908 | 8257.8 ± 0.8 | 192.9 ± 1.2 | −0.07 | −25.11 ± 0.09 | 237 ± 14 | 92.9 ± 0.8 | 23.1 ± 1.3 | 82.2 ± 2.0 | 9.35 ± 0.82 | 96.1 ±1.9 | 11.67 ±0.99 |
3091 | 5558.5 ± 0.6 | 209.9 ± 1.2 | −0.04 | −23.08 ± 0.18 | 156 ± 10 | 67.1 ± 0.6 | 25.4 ± 1.7 | 58.3 ± 1.4 | 4.60 ± 0.66 | 68.8 ±0.8 | 7.03 ±0.65 |
3140 | 4622.4 ± 0.4 | 352.5 ± 0.9 | −0.04 | −24.51 ± 0.09 | 209 ± 12 | 52.1 ± 0.4 | 14.4 ± 0.8 | 54.1 ± 0.9 | 6.14 ± 0.66 | 55.4 ±1.1 | 3.03 ±0.87 |
3701 | 2925.4 ± 0.6 | 91.0 ± 1.2 | −0.03 | −21.95 ± 0.22 | 124 ±9 | 56.1 ± 0.7 | 26.9 ± 2.0 | 50.6 ± 3.3 | 19.82 ± 2.67 | 57.9 ±1.7 | 17.45 ±1.49 |
3997 | 5943.3 ± 0.7 | 32.5 ± 1.2 | −0.05 | −23.01 ± 0.22 | 154 ± 11 | 68.2 ± 0.9 | 26.2 ± 1.9 | 63.8 ± 1.8 | 7.68 ± 0.87 | 71.0 ±1.4 | 11.64 ±1.02 |
4036 | 3466.2 ± 0.3 | 195.4 ± 0.8 | −0.03 | −23.96 ± 0.10 | 187 ± 11 | 52.6 ± 0.5 | 16.3 ± 1.0 | 48.7 ± 0.7 | 12.90 ± 0.70 | 53.3 ±1.6 | 13.59 ±2.73 |
4107 | 3507.6 ± 0.4 | 290.1 ± 0.6 | −0.03 | −23.37 ± 0.12 | 166 ± 10 | 67.7 ± 0.4 | 24.1 ± 1.5 | 63.8 ± 0.9 | 9.67 ± 0.58 | 68.4 ±0.9 | 9.08 ±0.62 |
4256 | 5248.2 ± 0.7 | 290.5 ± 1.0 | −0.04 | −24.81 ± 0.08 | 223 ± 13 | 74.2 ± 1.1 | 19.5 ± 1.1 | 63.0 ± 1.4 | 9.27 ± 0.91 | 84.8 ±2.8 | 17.94 ±1.53 |
4368 | 3876.2 ± 0.6 | 128.1 ± 0.6 | −0.03 | −23.29 ± 0.12 | 163 ± 10 | 116.1 ± 0.4 | 45.3 ± 3.3 | 113.1 ± 1.7 | 15.44 ± 0.68 | 117.0 ±1.3 | 13.28 ±0.72 |
4380 | 7481.3 ± 0.7 | 29.1 ± 1.8 | −0.06 | −23.98 ± 0.13 | 188 ± 12 | 46.0 ± 0.5 | 14.2 ± 0.9 | 36.0 ± 2.0 | 4.89 ± 1.21 | 42.2 ±1.5 | 4.04 ±1.68 |
4458 | 4751.7 ± 1.1 | 289.7 ± 0.9 | −0.04 | −25.29 ± 0.08 | 246 ± 14 | 140.1 ± 1.7 | 34.8 ± 2.2 | 117.9 ± 1.7 | 3.98 ± 0.68 | 138.0 ±3.6 | 0 |
4555 | 4243.9 ± 0.5 | 92.9 ± 0.4 | −0.04 | −23.84 ± 0.10 | 183 ± 11 | 115.9 ± 0.9 | 39.3 ± 2.6 | 109.9 ± 0.8 | 9.04 ± 0.40 | 114.5 ±1.3 | 3.55 ±0.84 |
4622 | 12 831.9 ± 1.1 | 118.3 ± 1.4 | −0.10 | −24.95 ± 0.12 | 229 ± 14 | 89.2 ± 0.7 | 22.9 ± 1.4 | 83.6 ± 3.5 | 5.68 ± 0.90 | 88.7 ±1.2 | 6.77 ±1.07 |
6903 | 1891.7 ± 1.2 | 143.0 ± 3.1 | −0.02 | −22.63 ± 0.20 | 143 ± 10 | 76.6 ± 1.3 | 32.4 ± 2.5 | 62.1 ± 8.7 | 17.55 ± 4.62 | 87.7 ± 18.2 | 34.26 ± 11.57 |
6918 | 1112.2 ± 0.3 | 191.6 ± 0.5 | −0.01 | −22.90 ± 0.23 | 151 ± 11 | 92.8 ± 0.4 | 38.0 ± 3.1 | 92.2 ± 0.3 | 10.01 ± 0.22 | 95.3 ±0.8 | 8.87 ±0.45 |
7244 | 4361.1 ± 0.5 | 149.8 ± 1.9 | −0.04 | −22.24 ± 0.21 | 132 ±9 | 38.2 ± 0.6 | 16.8 ± 1.2 | 25.8 ± 2.6 | 12.35 ± 2.87 | 37.4 ±2.1 | 20.02 ±2.40 |
7917 | 6998.1 ± 0.9 | 220.5 ± 0.8 | −0.06 | −25.35 ± 0.06 | 249 ± 14 | 129.8 ± 0.9 | 31.5 ± 1.9 | 120.7 ± 1.8 | 11.89 ± 0.72 | 118.1 ±7.1 | 10.40 ±2.49 |
8196 | 8336.9 ± 0.9 | 90.5 ± 1.1 | −0.07 | −25.36 ± 0.07 | 249 ± 14 | 69.0 ± 0.8 | 16.1 ± 0.9 | 60.6 ± 1.5 | 4.71 ± 0.92 | 60.8 ±2.9 | 2.99 ±1.27 |
9177 | 8866.6 ± 0.9 | 244.5 ± 0.7 | −0.08 | −24.50 ± 0.13 | 209 ± 13 | 135.4 ± 0.8 | 40.4 ± 2.7 | 134.6 ± 1.9 | 7.17 ± 0.57 | 143.0 ±1.3 | 9.17 ±0.89 |
9837 | 2654.9 ± 0.5 | 310.9 ± 1.0 | −0.03 | −22.71 ± 0.18 | 145 ±9 | 75.4 ± 0.5 | 31.3 ± 2.2 | 70.1 ± 3.4 | 16.05 ± 1.67 | 75.0 ±1.2 | 14.29 ±0.77 |
9965 | 4527.1 ± 0.4 | 203.2 ± 1.5 | −0.04 | −23.61 ± 0.11 | 174 ± 10 | 37.3 ± 0.6 | 12.4 ± 0.7 | 31.0 ± 1.2 | 7.32 ± 1.13 | 39.9 ±0.9 | 9.33 ±1.11 |
11 318 | 5884.5 ± 0.4 | 348.7 ± 1.7 | −0.05 | −24.67 ± 0.08 | 217 ± 12 | 21.9 ± 0.6 | 5.8 ± 0.4 | 20.9 ± 0.8 | 6.87 ± 1.48 | 25.8 ±1.6 | 14.37 ±2.52 |
12 391 | 4880.5 ± 0.5 | 38.6 ± 0.9 | −0.04 | −23.54 ± 0.12 | 172 ± 10 | 83.7 ± 0.7 | 29.2 ± 1.8 | 73.0 ± 1.6 | 11.20 ± 0.81 | 87.0 ±2.2 | 16.55 ±1.33 |
Notes. Numbers in italics are used to calculate iTF. (1) UGC number; (2) weighted-average heliocentric systemic velocity; (3) position angle of the receding side of the kinematic major axis; (4) k-correction used to calculate MK following κK = (1 + α)2.5log (1 + z) with α = 1.25 for the K-band according to Bershady (1995); (5) absolute, total K-band magnitude based on Table 1 with A and κK applied; (6) amplitude of the flat part of the rotation curve as predicted by the Tully-Fisher relation; (7) weighted-average projected rotation velocity derived from the Hα, [Oiii] and HI position–velocity diagrams; (8) derived inclination based on the Tully-Fisher relation; (9) asymptotic maximum rotational velocity of the tanh-model fitted to the stellar data; (10) scale-radius of the tanh-model fitted to the stellar data; (11) and (12) identical to (9) and (10) but then for the [Oiii] gas.
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