Table 11
Mean disk dust masses and mean stellar masses for the samples from five star-forming regions plotted in Fig. 5 and discussed in the text.
| Region/Sample | < Mdust > | σ(a) | < M∗ > | σ (a) | Age |
|---|---|---|---|---|---|
| (M⊕) | (M⊕) | (M⊙) | (M⊙) | (Myr) | |
| M17 | 1.7 | 0.82 | 6.5 | 2.3 | 0.6±0.3 |
| Upper Sco | 3.9 | 15 | 0.33 | 0.29 | 5–11 |
| ONC (b) | 8.2 | 14 | 0.78 | 2.3 | ∼1 |
| Lupus | 17 | 28 | 0.45 | 0.50 | 1–3 |
| Herbig sample (c) | 40 | 48 | 2.0 | 0.38 | 7±3 |
Notes. (a) Standard deviation of the averaged values. (b) Orion Nebula Cluster sample from Eisner et al. (2018), not plotted in Fig. 5. (c)The main sample from Stapper et al. (2022) (blue marks in Fig. 5), excluding the higher mass exceptions (gray marks in Fig. 5; see also Sect. 5.2.2).
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