Table 1
Summary of the properties of the different MCs studied in this paper, as well as their division into patches at different sampling.
| Region | Dist. | Coord. | # patches with resolution | References | |||||
|---|---|---|---|---|---|---|---|---|---|
| d (pc) | l(°) | b(°) | Total | 6″ | 9″ | 12″ | 18″ | ||
| Aquila | 436 | 28 | 4 | 57 | 36 | 16 | 4 | 1 | 1 |
| Chamaeleon I | 210 | 296 | −16 | 28 | 20 | 6 | 2 | 0 | 2 |
| Chamaeleon II III | 160 | 302 | −16 | 43 | 32 | 8 | 3 | 0 | 2 |
| Corona Australis | 160 | 0 | −19 | 44 | 34 | 7 | 3 | 0 | 2 |
| IC 5146 | 750 | 94 | −5 | 4 | 4 | 0 | 0 | 0 | 2 |
| Lupus I | 182 | 339 | 17 | 17 | 12 | 4 | 1 | 0 | 3 |
| Musca | 200 | 301 | −9 | 6 | 6 | 0 | 0 | 0 | 4 |
| Ophiuchus | 139 | 353 | 17 | 61 | 42 | 12 | 6 | 1 | 5 |
| Orion B | 450 | 205 | −14 | 88 | 61 | 19 | 7 | 1 | 2, 6 |
| Perseus | 285 | 159 | −20 | 44 | 32 | 10 | 2 | 0 | 2 |
| Pipe Nebula | 180 | 359 | 6 | 23 | 18 | 5 | 0 | 0 | 2 |
| Polaris Flare | 400 | 123 | 26 | 50 | 36 | 9 | 4 | 1 | 2, 6 |
| Serpens | 436 | 31 | 4 | 46 | 33 | 9 | 4 | 0 | 1 |
| Taurus | 145 | 170 | −16 | 40 | 30 | 6 | 4 | 0 | 7 |
Notes. References in the rightmost column are for the distance estimates. These can vary by several tens of percentage depending on the line of sight. Such variability along with uncertainties are given in the references quoted. (1) Ortiz-León et al. (2018); (2) Zucker et al. (2020); (3) Galli et al. (2013); (4) Knude & Hog (1998); (5) Mamajek (2008); (6) Schlafly et al. (2014); (7) Yan et al. (2019).
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