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Table B.1

Parameters describing the gas distribution of the Bonnor-Ebert spheres.

M NH ρC R AV AV AV AV AV AV
(M) (H/cm2) (H/cm3) (pc) DHGL accretion 0% 10% 25% 40%

0.5 5 × 1022 780 072 0.025 25.1 27.3 23.0 24.0 25.9 27.9
0.6 4 × 1022 541 717 0.03 20.9 22.8 19.2 20.0 21.6 23.3
0.7 3.5 × 1022 397 996 0.035 17.9 19.5 16.5 17.2 18.5 19.9
0.8 3 × 1022 304 716 0.04 15.7 17.1 14.4 15.0 16.2 17.5
0.9 2.7 × 1022 240 762 0.045 13.9 15.2 12.8 13.4 14.4 15.5
1 2.5 × 1022 195 018 0.05 12.5 13.7 11.5 12.0 12.9 14.0
2 1.2 × 1022 48 755 0.1 6.3 6.8 5.8 6.0 6.5 7.0
5 5 × 1021 7801 0.25 2.5 2.7 2.3 2.4 2.6 2.8
10 2.5 × 1021 1950 0.5 1.2 1.4 1.2 1.2 1.3 1.4
20 1.2 × 1021 488 1.0 0.6 0.7 0.6 0.6 0.7 0.7
50 5 × 1020 78 2.5 0.3 0.3 0.2 0.2 0.3 0.3
100 2.5 × 1020 20 5.0 0.1 0.1 0.1 0.1 0.1 0.1

Notes. M is the the cloud mass in units of solar masses, NH is the hydrogen column density at the centre of the cloud, ρC is the central hydrogen density, R is the external radius of the sphere, and AV is the visual extinction at the centre of the cloud, which depends on the grain populations considered (labels are the same as in Table 2).

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