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Table 7
Best-fit parameters of the 3D geometry.
| Region | Lyα contribution | UV contribution | v exp | N HI | τLyα (E(B − V)) | b (temperature) |
| km s-1 | cm-2 | km s-1 (K) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
|
|
||||||
| Galaxy disk | 0% | 80% | 100 | 4 ×1020 | 3.50 (0.34) | 12.8 (10 000) |
| Halo 1 | 55% | 9% | 180 | 4 ×1019 | 1.10 (0.09) | 22.8 (31 000) |
| Halo 2 | 45% | 11% | 100 | 3 ×1019 | 1.20 (0.11) | 22.8 (31 000) |
Notes.For each component of our 3D geometry, we list the photometric properties in Cols. 2 and 3 and the derived physical parameters (vexp, 
, τLyα, b) in Cols. 4−7.
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