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Table A.1
Same as Table 1 but the radii correspond to deconvolved CO radii and the fluxes have been extracted without the local background subtraction.
| Name | Radius | S 160 μm | S 870 μm | S1.2 mm | S3 cm | S6 cm | |||
| pc | Jy | mJy | mJy | mJy | mJy | ||||
|
|
|||||||||
| LIRS49 | 10.6 | 39.5 ± 3.4 | 2241 ± 266 | 457 ± 91 | 36 ± 5 | 36 ± 4 | |||
| LIRS36 | 13.4 | 24.5 ± 4.6 | 1551 ± 140 | 462 ± 90 | 80 ± 30 | 74 ± 21 | |||
| SMCB1#1 | 4.8 | 3.9 ± 0.9 | 507 ± 120 | 215 ± 63 | < 10 | < 5 | |||
| SMCB1#2 | 9.5 | 10.1 ± 2.1 | 1252 ± 185 | 265 ± 71 | 21 ± 6 | 24 ± 3 | |||
| SMCB1#3 | NaN | 5.4 ± 1.4 | 589 ± 99 | 69 ± 19 | 12 ± 4 | 13 ± 3 | |||
| Hodge 15 | 12.5 | 0.68 ± 0.35 | 467 ± 83 | 176 ± 43 | 2.3 ± 1.2 | 5 ± 2 | |||
| SMCB2 South1 | 8.4, NaN, 7.2 | 45 ± 9 | 2603 ± 557 | 917 ± 187 | 114 ± 20 | 105 ± 25 | |||
| SMCB2 North2 | 14.8, NaN | 43 ± 6 | 2137 ± 330 | 577 ± 165 | 79 ± 15 | 87 ± 10 | |||
| SMCB2#5 | 7.6 | 6.3 ± 1.5 | 170 ± 116 | 71 ± 44 | 27 ± 17 | 27 ± 17 | |||
Notes. When the observed radius of the cloud was lower than the beam, the deconvolved radius was set to NaN and we used the observed CO radius to compute masses instead.
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