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Table 1
Physical quantities and notation of the applied models.
| Molecular cloud models (mass) | |||||
|---|---|---|---|---|---|
| Cloud mass [M⊙] | 104 | 105 | 106 | 107 | |
| Notation | M4 | M5 | M6 | M7 | |
| Cluster models (mass) | |||||
| Cluster mass [M⊙] | 103 | 104 | 105 | 106 | 107 |
| Cluster luminosity [L⊙] | 1.02 × 106 | 1.02 × 107 | 1.02 × 108 | 1.02 × 109 | 1.02 × 1010 |
| Notation | C3 | C4 | C5 | C6 | C7 |
| Cluster models (concentration) | |||||
| FWHM [pc] | 0 | 0.1 | 1 | 2 | 4 |
| Notation | F0 | F0.1 | F1 | F2 | F4 |
| Dust models (grain size) | |||||
| amax [μm] | 0.02 | 0.2 | 2.0 | 20.0 | 200.0 |
| Notation | D1 | D2 | D3 | D4 | D5 |
Notes. Our clouds are spherically symmetric and follow a Plummer-like density profile (Eq. (1)) with a core radius of 1% of the outer radius, Rc = 0.01Rout. The standard cloud radiusis Rout = 5 pc, but we also consider values of 20 and 150 pc for selected cases.
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