Table A.1.
Kinematic parameters
| Population | Relative density | Scale-height | Scale-length | < U> | < V> | < W> | σU | σV | σW |
|---|---|---|---|---|---|---|---|---|---|
| (kpc) | (kpc) | (km s−1) | (km s−1) | (km s−1) | (km s−1) | (km s−1) | (km s−1) | ||
| Thin disc | 0.9 | 0.3 | 2.6 | 0 | 236 | 0 | 39 | 20 | 20 |
| Thick disc | 0.08 | 0.9 | 2.0 | 0 | 206 | 0 | 63 | 39 | 39 |
| Halo | 0.02 | – | – | 0 | 0 | 0 | 141 | 106 | 94 |
Notes. We assumed that the thin and thick discs follow Gaussian velocity distributions, with means and standard deviations from Soubiran et al. (2003), and a halo component with velocity dispersion following Chiba & Beers (2000). We used the density fractions of Ramírez et al. (2013), and the scale-heights, scale-lengths, and halo power law are based on Bland-Hawthorn & Gerhard (2016).
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