Open Access
Table H.2.
For each one of the molecular clouds on the line of sight of HESS J1702-420: distance and density from (Lau et al. 2018), and proton energetics that would be necessary to power the observed VHE emission of HESS J1702-420B in each case.
| Near distance | nH | Wp(E > 1 GeV) |
|---|---|---|
| [kpc] | [ × 100 cm−3 ] | [erg] |
| 0.25 | 1.8 | 7.9 1045 |
| 0.5 | 5 | 1.1 1046 |
| 1.6 | 1 | 5.8 1047 |
| 2.6 | 3.3 | 4.7 1047 |
| 4 | 1.4 | 2.6 1048 |
| 5.1 | 0.5 | 1.2 1049 |
| 5.7 | 0.4 | 1.9 1049 |
| 6 | 0.2 | 4.1 1049 |
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