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Table 1
Molecular clouds in the Cygnus region.
| Name | 1[º] | Distance [kpc] | Distance ref | |
|---|---|---|---|---|
| A | Foreground Rift | 74–86 | 0.7−1.1 | Zhang et al. (2024) |
| B | Cygnus North-West | 79.5–81 | ~1 | Zhang et al. (2024) |
| C | Cygnus 1.3 North | 80–83.5 | 1.3−1.4 | Zhang et al. (2024) |
| D | Cygnus 1.3 South | 77–80 | 1.2−1.3 | Zhang et al. (2024) |
| E | Cygnus North Filament | 80.5–82 | 1.4−1.5 | Rygl et al. (2012) |
| F | Cygnus Central Clumps | 79–81 | 1.6−1.8 | Orellana et al. (2021); Xu et al. (2013b) |
| G | Cygnus West | 78–80 | >1.4 | |
| H | Cygnus SFR South | 77–80 | >1.4 | |
| J | Cygnus South Filament | 77–79 | >1.4 | |
| K | Cygnus Far South | 76–78 | 1.6−1.8 | Schneider et al. (2007) |
Notes. Section 4 describes the procedure by which the clouds were identified. Figure 5 shows a map of the clouds. The specific distance and mass estimates assumed in the calculation of the γ-ray flux are provided in https://doi.rg/18.17617/3.G9LUS1.
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