Table 3
Properties of the nuclei.
| nucleus | v max | σ | n | ϵ | r eff | r kin | L K | M dyn | Mdyn/LK |
| [km s-1] | [km s-1] | [pc] | [pc] | [L⊙] | [L⊙] | [L⊙/M⊙] | |||
|
|
|||||||||
| North | 205 | 200 | 2.8 | 0.3 | 490 | 265 | 1.1 × 109 | 2.5 × 109 | 5.0 |
| South | 300 | 220 | 2.8 | 0.35 | 180 | 290 | 5.9 × 109 | 1.3 × 1010 | 1.9 |
References. vmax is the peak measured stellar velocity, σ is the average/typical stellar dispersion (Sect. 2.1.4); n and reff are the Sérsic index and effective radius of the light profile (Sect. 7), ϵ is the ellipticity (Sect. 5), rkin is the extent to which rotation is seen, LK the total K-band luminosity (Sect. 4), and Mdyn the dynamical mass as derived from the Jeans modelling (Sect. 7).
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