Table 1.
Data adopted for the dwarf models.
| Dwarf | LV (105 L⊙) | b (kpc) | xMW (kpc) | yMW (kpc) | zMW (kpc) | r⊙ (kpc) |
|---|---|---|---|---|---|---|
| Draco | 2.7 | 0.196 | −4.3 | 62.2 | 43.2 | 76 ± 6 |
| Ursa Minor | 2 | 0.28 | −22.2 | 52 | 53.5 | 76 ± 3 |
| Sculptor | 14 | 0.26 | −5.2 | −9.8 | −85.3 | 86 ± 6 |
| Sextans | 4.1 | 0.682 | −36.7 | −56.9 | 57.8 | 86 ± 4 |
| Carina | 2.4 | 0.241 | −25 | −95.9 | −39.8 | 105 ± 6 |
| Fornax | 140 | 0.668 | −41.3 | −51 | −134.1 | 147 ± 12 |
| Leo II | 5.9 | 0.151 | −77.3 | −58.3 | 215.2 | 233 ± 14 |
| Leo I | 34 | 0.246 | −123.6 | −119.3 | 191.7 | 254 ± 15 |
Notes. Columns: (1) dwarf name; (2) V-band luminosity used to determine the stellar mass; (3) scale length used in the Plummer model for the stellar distribution (LV and b are from McConnachie 2012 and references therein); (4–7) coordinates of the Milky Way centre in the Cartesian system where the dwarf is at the origin and the heliocentric distance (from Pawlowski & Kroupa 2013; McConnachie 2012; see Sect. 4.3).
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.