Table 3
Fractions f90 and f60 of the area of the E − Lz space dominated by accreted stars, relative to the area occupied by the whole distribution of halo stars (see Sect. 3.1.3 for their definition), in the case of the 1 × (1:10) simulation.
| R sun | Volume # | f 90 | f 60 |
|
|
|||
| 8. | 1 | 0.16 | 0.25 |
| 8. | 2 | 0.16 | 0.25 |
| 8. | 3 | 0.18 | 0.28 |
| 8. | 4 | 0.15 | 0.26 |
| 8. | 5 | 0.13 | 0.22 |
| 8. | 6 | 0.16 | 0.26 |
| 8. | 7 | 0.16 | 0.27 |
| 8. | 8 | 0.14 | 0.25 |
| 12. | 1 | 0.21 | 0.33 |
| 12. | 2 | 0.20 | 0.31 |
| 12. | 3 | 0.27 | 0.40 |
| 12. | 4 | 0.21 | 0.32 |
| 12. | 5 | 0.19 | 0.30 |
| 12. | 6 | 0.22 | 0.36 |
| 12. | 7 | 0.21 | 0.34 |
| 12. | 8 | 0.22 | 0.35 |
Notes. These fractions are reported here for all the different “solar vicinity” volumes shown in Fig. 5.
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