Table 3.
Main kinematical parameters derived from the stellar modelling and for the individual components detected in the gas modelling of the Hα line for all the cubes.
| Galaxy | PA⋆ | Δv⋆ |
 |
PAgas, P | Δvgas, P |
 |
⟨vgas, S⟩ |
 |
Broad | FWHM |
|---|---|---|---|---|---|---|---|---|---|---|
| (°) | (km s−1) | (km s−1) | (°) | (km s−1) | (km s−1) | (km s−1) | (km s−1) | (Y or N) | (km s−1) | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| NGC 0266 | 121 ± 7 | 172 | 182 ± 14 | – | – | 173 ± 28 | – | – | N | – |
| NGC 0315 | – | – | 335 ± 13 | 225 ± 8 | 156 | 195 ± 38 | 96 ± 77 | 480 ± 120 | Y | 2655 ± 360 |
| NGC 3226 | 49 ± 4 | 106 | 210 ± 17 | 19 ± 4 | 219 | 136 ± 55 | −91±27 | 262 ± 42 | Y | 2305 ± 153 |
| NGC 3245 | 178 ± 3 | 144 | 245 ± 18 | 174 ± 6 | 232 | 154 ± 46 | −214 ± 142 | 198 ± 173 | N | – |
| NGC 4278( † ) | 20 ± 1 | 104 | 336 ± 35 | 46 ± 10 | 240 | 146 ± 23 | 82 ± 150 | 49 ± 27 | ||
| NGC 4438 | 27 ± 2 | 111 | 148 ± 7 | 28 ± 6 | 154 | 99 ± 28 | −8 ± 35 | 256 ± 57 | [Y] | [1980 ± 350] |
| NGC 4750 | 210 ± 10 | 97 | 134 ± 7 | – | – | 153 ± 29 | −92 ± 50 | 297 ± 41 | Y | 2188 ± 300 |
| NGC 5055 | 99 ± 4 | 79 | 50 ± 4 | 107 ± 11 | 126 | 69 ± 26 | – | – | N | – |
Notes. Columns indicate: (1) object, ( † )indicates that the values correspond to the [O III] line; (2) major axis position angle of the stellar velocity maps using the receding sides as reference; (3) semi-amplitude velocity of the stellar maps; (4) central velocity dispersion in the PSF region of the stellar maps; (5) position angle for the major axis of the primary component of the ionised gas; (6) and (7) semi-amplitude velocity and central velocity dispersion (in the PSF region) of the primary component of the ionised gas; (8) and (9) average velocity and velocity dispersion integrated in the PSF region for the secondary component of the ionised gas; (10) indicates if there is or not a broad component associated with the BLR detected in the Balmer lines and (11) the FWHM of that component. For all columns, the reported errors are 1σ values. [] indicates that the BLR fit is not well constrained.
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