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Table 5

Source parameters of the six W33 clumps derived from continuum observations at 870 μm.

Clump r aperture r equiv F peak a F 24″ a F source a T cold L bol β M source N H2,peak N H2,24″ N H2,source
()/(pc) ()/(pc) (Jy) (Jy) (Jy) (K) (103 L) (103M) (1023 cm-2) (1023 cm-2) (1022 cm-2)

W33 Main1 58/0.7 53/0.6 3.4 4.0 21.3 28.6 ± 5.6 11 1.4 ± 0.5 0.5 ± 0.3 0.9 ± 0.2 0.7 ± 0.2 2.4 ± 0.7
W33 A1 40/0.5 32/0.4 3.2 3.9 8.6 25.0 ± 7.3 6 1.8 ± 0.9 0.4 ± 0.5 1.7 ± 0.6 1.2 ± 0.4 5.4 ± 2.3
W33 B1 49/0.6 48/0.6 3.1 3.4 14.8 38.6 ± 11.4 16 1.3 ± 0.5 0.2 ± 0.1 0.5 ± 0.2 0.4 ± 0.1 1.2 ± 0.5
W33 B 75/0.9 86/1.0 5.4 6.6 60.7 26.5 ± 3.9 22 1.6 ± 0.4 1.9 ± 1.1 2.1 ± 0.5 1.6 ± 0.4 3.7 ± 0.9
W33 A 82/1.0 128/1.5 9.2 11.2 153.4 28.6 ± 5.3 41 1.4 ± 0.5 3.4 ± 2.3 2.5 ± 0.6 2.0 ± 0.6 3.0 ± 0.9
W33 Main 102/1.2 126/1.5 36.5 43.9 383.4b 42.5 ± 12.6 449 1.2 ± 0.4 4.0 ± 2.5 4.6 ± 1.6 3.6 ± 1.4 3.8 ± 1.5

Notes. Column 1: clump name; Col. 2: radius of the aperture, used for photometry; Col. 3: equivalent radius, characterising the clump area at the 5σ level; Col. 4: peak flux density; Col. 5: flux density, integrated over an area of 24 × 24; Col. 6: flux density of the whole clump; Col. 7: temperature of the cold component; Col. 8: bolometric luminosity; Col. 9: spectral emissivity index β; Col. 10: total mass of the clump; Col. 11: H2 peak column density; Col. 12: H2 column density over an area of 24× 24; Col. 13: H2 column density of the whole clump.

(a)

Assumed uncertainty: 15%.

(b)

~18 Jy from free-free emission.

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