Table 4
Magnetic field strength for the different objects, derived from equipartition with turbulent pressure is listed.
| i | Name | Δv | Beq | Ref. |
|---|---|---|---|---|
| (km s−1) | (mG) | |||
| 1 | Sgr C | 6.5 | 0.6 | 1 |
| 2 | SgrA* | – | 6.5 × 103 | 5 |
| 3 | inner 5 pc | – | 8.4 | 2 |
| 4 | 20 km s−1 | 10.2 | 0.9 | 2 |
| 5 | 50 km s−1 | 13.9 | 1.3 | 2 |
| 6 | Dust Ridge A | 6.5 | 0.5 | 3 |
| 7 | Dust Ridge B | 6.8 | 0.4 | – |
| 8 | Dust Ridge C | 6.8 | 0.4 | – |
| 9 | Dust Ridge D | 7.0 | 0.4 | 3 |
| 10 | Dust Ridge E | 6.7 | 0.7 | 3 |
| 11 | Dust Ridge F | 7.2 | 0.9 | 3 |
| 12 | Sgr B2 | – | 1.3 | 4 |
| 13 | Sgr D | 2.5 | 0.2 | 1 |
Notes. Magnetic field results for the inner 5 pc and Sgr B2 are adopted from observations. For dust ridge B and C, the average velocity dispersion in the dust ridge is used.
References. 1 = Kauffmann et al. (2017b), 2 = Plante et al. (1994), 3 = Walker et al. (2015), 4 = Crutcher et al. (1996), 5 = Eatough et al. (2013).
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