Table 2
Properties of observed clusters taken from Lada & Lada (2003) and Pfalzner (2009).
| ID | Age | Mc | reff |
|
|
|||
| GGD 12–15a | 4 | 73 | 0.615 |
| NGC 2282b | 5 | 170 | 0.8 |
| NGC 2024c | 0.3 | 180 | 0.44 |
| IC 348d | 1.3 + 1.6 | 160 | 0.5 |
| L 1641-Ce | 0.1 | 27 | 0.155 |
| NGC 2068f | 2 | 110 | 0.43 |
| NGC 2071f | 2 | 60 | 0.29 |
| NGC 1333g | 1 | 79 | 0.245 |
| Mon R2h | 0.8 | 340 | 0.925 |
| ONC | 1 | 1100 | 1.9 |
| Cyg OB2i | 1–4 | 4.4 | 5.2 |
| NGC 6611i | 1–5 | 4.4 | 5.9 |
| NGC 2244i | 1–3 | 3.9 | 5.6 |
| IC 1805i | 1–3 | 4.2 | 7.1 |
| Ori Ibi | 1.7 | 3.6 | 6.3 |
| NGC 7380i | 2 | 3.8 | 6.5 |
| Ori Ici | 4.6 | 3.8 | 12.5 |
| Ori Iai | 11.4 | 3.7 | 16.6 |
| U Scoi | 5–11 | 3.5 | 14.2 |
| Lower Cen-Cruxi | 11–12 | 3.3 | 15.0 |
| Upper Cen-Lup2i | 14–15 | 3.6 | 22.1 |
| I Lac 2i | 12–16 | 3.4 | 20.7 |
Notes. No errors are included in Table 2, because the embedded nature leads to intrinsically uncertainity in the mass estimate.
Reference. Cluster ages added from the following sources:
Maaskant et al. (2011);
Horner et al. (1997);
Eisner & Carpenter (2003);
Herbig (1998);
Allen & Davies (2008);
Flaherty & Muzerolle (2008);
Raga et al. (2013);
Pfalzner (2009, and references therein).
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