Table 1
Data relevant for the TFRs discussed in this paper.
| ID | D | Method | i | Δi | v circ | Δvcirc | log MHI | log Lr |
|
|
| (Mpc) | (deg) | (deg) | (km s-1) | (km s-1) | (M⊙) | L ⊙ | M ⊙ / L ⊙ r | M ⊙ / L ⊙ r | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
|
|
||||||||||
| NGC 2685 | 16.7 | c | 65 | 4 | 144 | 10 | 9.33 | 9.857 | 0.455 | 0.620 |
| NGC 2824 | 40.7 | c | 65 | 8 | 162 | 10 | 7.59 | 9.889 | 0.628 | 0.343 |
| NGC 2859 | 27 | v | 35 | 5 | 215 | 41 | 8.46 | 10.404 | 0.568 | 0.732 |
| NGC 2974 | 20.9 | v | 60 | 2 | 310 | 10 | 8.74 | 10.152 | 0.981 | 0.787 |
| NGC 3522 | 25.5 | v | 41 | 2 | 121 | 8 | 8.47 | 9.600 | 0.705 | 0.648 |
| NGC 3626 | 19.5 | v | 54 | 1 | 169 | 8 | 8.94 | 10.102 | 0.437 | 0.261 |
| NGC 3838 | 23.5 | c | 66 | 8 | 159 | 14 | 8.38 | 9.772 | 0.589 | 0.694 |
| NGC 3941 | 11.9 | v | 57 | 1 | 148 | 8 | 8.73 | 9.940 | 0.400 | 0.693 |
| NGC 3945 | 23.2 | v | 57 | –5, +1 | 237 | 13 | 8.85 | 10.394 | 0.628 | 0.760 |
| NGC 3998 | 13.7 | v | 66 | 2 | 246 | 20 | 8.45 | 9.967 | 0.971 | 0.818 |
| NGC 4203 | 14.7 | c | 30 | 3 | 197 | 35 | 9.15 | 10.067 | 0.537 | 0.827 |
| NGC 4262 | 15.4 | v | 67 | –8, +1 | 198 | 10 | 8.69 | 9.726 | 0.753 | 0.782 |
| NGC 4278 | 15.6 | v | 45 | –2, +5 | 256 | 26 | 8.80 | 10.247 | 0.829 | 0.846 |
| NGC 5582 | 27.7 | v | 50 | 2 | 258 | 10 | 9.65 | 10.140 | 0.722 | 0.752 |
| NGC 6798 | 37.5 | v | 52 | 2 | 190 | 8 | 9.38 | 10.028 | 0.660 | 0.684 |
| UGC 6176 | 40.1 | v | 47 | –2, +6 | 144 | 14 | 9.02 | 9.751 | 0.685 | 0.328 |
Notes. List of the galaxies where the circular velocities at large radii are derived from the H i kinematics. Column (1): the name is the galaxy designation. Column (2): galaxy distance as listed in Cappellari et al. (2011). Column (3): c indicates that the circular velocity is based on an analysis of the full data cube, whereas v indicates a velocity-field based circular velocity. Columns (4) and (5): inclination angle and uncertainty. Columns (6) and (7): circular velocity and uncertainty. Column (8): H i-mass (from Serra et al. 2012). Columns (9): r-band luminosity (from Cappellari et al. 2013b). Column (10): r-band mass-to-light ratios from stellar dynamics (from Cappellari et al. 2013b) and Col. (11): r-band mass-to-light ratios from star formation histories (from Cappellari et al. 2013a).
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.