Table A.1
Parameters of CMFGEN models of Mercer 30 cluster members that are not crucial for our discussions.
| ID | νsini a | ζ mac a | ξ mic a | ν∞ a | β | Ṁ [M⊙ yr-1] | C L 1 a | C L 2 a,b | C L 3 a,b | C L 4 b | Z C c | Z N c | Z O c | |
|
|
||||||||||||||
| Mc30-1 | 65 | 65 | 15 | 1400 | 1.35 | 2.2 × 10-5 | 0.100 | 320 | 75 | 0.10 | ≤40 | 5.0 | ≤0.8 | |
| Mc30-2 | 10 | 85 | 15 | 600 | 2.00 | 1.1 × 10-5 | 0.250 | 10 | 60 | 0.15 | 0.7 | 11.4 | 3.1 | |
| Mc30-3 | 65 | 65 | 15 | 2500 | 1.05 | 7.3 × 10-7 | 0.100 | 50 | 75 | 0.10 | 1.5 | 1.0 | 7.0 | |
| Mc30-5 | 50 | 50 | 12 | 2500 | 0.80 | 1.2 × 10-6 | – No clumping – | 1.0 | 0.8 | 2.5 | ||||
| Mc30-6a | 35 | 110 | 20 | 1600 | 1.75 | 1.2 × 10-5 | 0.100 | 65 | 100 | 0.20 | ≤0.6 | 4.0 | ≤3.0 | |
| Mc30-6b | 100 | 50 | 17 | 1600 | 0.90 | 9.4 × 10-6 | 0.100 | 135 | 75 | 0.10 | ≤0.8 | 4.0 | ≤3.0 | |
| Mc30-7 | 180 | 65 | 25 | 2000 | 1.00 | 2.0 × 10-5 | 0.075 | 140 | 5 | 0.10 | ≤0.2 | 10.0 | ≤2.0 | |
| Mc30-8 | 65 | 65 | 25 | 1200 | 1.07 | 3.6 × 10-5 | 0.250 | 135 | 170 | 1.00 | ≤0.2 | 19.5 | ≤0.6 | |
| Mc30-9 | 65 | 65 | 15 | 2500 | 0.80 | 4.3 × 10-6 | – No clumping – | 1.4 | 0.8 | 4.0 | ||||
| Mc30-10 | 65 | 65 | 20 | 2500 | 1.25 | 2.7 × 10-6 | – No clumping – | 0.8 | 1.9 | 3.2 | ||||
| Mc30-11 | 150 | 65 | 20 | 2500 | 1.05 | 4.2 × 10-6 | – No clumping – | 1.0 | 1.0 | 4.0 | ||||
| Mc30-13 | 130 | 65 | 25 | 2500 | 1.50 | 2.7 × 10-6 | – No clumping – | 0.4 | 1.5 | 5.2 | ||||
| Mc30-18 | 120 | 100 | 14 | 2500 | 0.80 | 3.1 × 10-6 | 0.300 | 150 | 75 | 0.30 | 0.4 | 1.2 | 1.5 | |
| Mc30-19 | 65 | 65 | 17 | 2500 | 1.05 | 2.0 × 10-6 | – No clumping – | 0.9 | 3.5 | 4.6 | ||||
| Mc30-22 | 50 | 115 | 10 | 2500 | 0.80 | 5.4 × 10-7 | – No clumping – | 1.5 | 0.8 | 4.0 | ||||
Notes.
The coefficients for the clumping law of Najarro et al. (2009) are used, however when CL4 = CL1 the clumping law of Hillier & Miller (1999) is recovered with a = CL1 and b = CL2 (which occurs for the Mc30-1, Mc30-3, Mc30-6b, and Mc30-18 models).
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