Table 3
Mass estimates for the individual GMCs observed in the southwest region of the SMC.
| Name |  (12 K) |
(19 K) |
|
| 104 M⊙ | 104 M⊙ | ||
|
|
|||
| LIRS49 | 56 ± 5 | 31 ± 3 | 12.2 ± 0.5 |
| LIRS36 | 50 ± 5 | 23 ± 2 | 5.1 ± 0.5 |
| SMCB1#1 | 12 ± 2 | 5 ± 1 | 2.5 ± 0.2 |
| SMCB1#2 | 33 ± 7 | 18 ± 4 | 7.4 ± 1.4 |
| SMCB1#3 | 11 ± 4 | 6 ± 2 | 2.5 ± 0.2 |
| Hodge15 | 50 ± 12 | 17 ± 4 | 7.2 ± 0.4 |
| SMCB2 South | 65 ± 22 | 35 ± 12 | 14.4 ± 2.3 |
| SMCB2 North | 85 ± 11 | 46 ± 6 | 9.8 ± 1.9 |
| SMCB2#5 | 8 ± 6 | 4 ± 3 | 5.0 ± 0.3 |
Notes. The first two columns give the mass estimates computed from the LABOCA 870 μm emission for dust temperatures of 12 K and 19 K, respectively, while the third column lists the virial masses obtained from the CO line widths and the cloud radii.
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