Table 4.
Kinematic properties extracted from the DiskFit models for the H- and K-band velocity maps.
Name | ΔRAH | ΔDecH | PAH | iH | ϕH | ΔRAK | ΔDecK | PAK | iK | ϕK |
---|---|---|---|---|---|---|---|---|---|---|
(arcsec) | (arcsec) | (deg) | (deg) | (deg) | (arcsec) | (arcsec) | (deg) | (deg) | (deg) | |
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
NGC 2369 | −0.27 ± 0.03 | 0.52 ± 0.09 | 173 ± 1 | 63 ± 2 | ... | −0.16 ± 0.07 | 0.58 ± 0.05 | 172 ± 1 | 64 ± 2 | ... |
NGC 3110 | 0.08 ± 0.08 | 0.25 ± 0.08 | 168 ± 2 | 50 ± 7 | ... | −0.19 ± 0.04 | 0.28 ± 0.05 | 173 ± 1 | 57 ± 2 | ... |
NGC 3256 | −0.50 ± 0.18 | 0.60 ± 0.24 | 80 ± 2 | 18 ± 2 | ... | ... | ... | ... | ... | ... |
ESO 320-G030 | −0.04 ± 0.05 | −0.07 ± 0.06 | 129 ± 1 | 51 ± 2 | 97 ± 5 | −0.20 ± 0.03 | −0.05 ± 0.02 | 132 ± 1 | 43 ± 5 | 82 ± 7 |
IRAS F12115-4656 | ... | ... | ... | ... | ... | −0.31 ± 0.02 | −0.13 ± 0.03 | 124 ± 2 | 69 ± 3 | ... |
NGC 5135 | −0.94 ± 0.04 | −0.15 ± 0.06 | 8 ± 3 | 39 ± 6 | ... | −0.72 ± 0.15 | −0.19 ± 0.13 | 6 ± 2 | 18 ± 6 | ... |
IRAS F17138-1017 | −0.59 ± 0.05 | −0.21 ± 0.03 | 2 ± 3 | 61 ± 7 | 36 ± 8 | −0.48 ± 0.08 | −0.15 ± 0.08 | 6 ± 1 | 65 ± 2 | 36 ± 3 |
IC 4687 (†) | ... | ... | 40 ± 3 | 18 ± 4 | ... | ... | ... | 41 ± 3 | 18 ± 5 | ... |
NGC 7130 | 0.27 ± 0.08 | −0.17 ± 0.09 | 53 ± 1 | 18 ± 9 | ... | 0.01 ± 0.07 | 0.05 ± 0.06 | 45 ± 5 | 32 ± 13 | ... |
IC 5179 | −0.55 ± 0.37 | 0.21 ± 0.20 | 51 ± 2 | 70 ± 20 | ... | −0.55 ± 0.32 | 0.47 ± 0.26 | 52 ± 2 | 57 ± 17 | ... |
Notes. Columns (2), (3), (7), and (8): position of the kinematic centres (i.e. RA and Dec), as the distance from the photometric centre (see Table 3). Columns (4) and (9): position angle (PA), defined as the anti-clockwise angle from the north to the semi-major axis. Columns (5) and (10): inclination values, computed as cos i = b/a, where b/a is the minor-to-major axis ratio. Columns (6) and (11): orientation of the additional radial component (ϕ = PA-θb) for those objects that showed radially structured residuals, defined as from north to east. (†)For this object, we forced the kinematic centre to coincide with the photometric centre during the fit.
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