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Table 4

Physical properties of the 12CO clumps in 30 Dor.

ID L12CO R Mvir MgasCO$M^{\rm CO}_{\mathrm{gas}}$ ΣH2 M v i r M gas CO $M^{\rm CO}_{\mathrm{gas}}$
(K km s-1 pc-2) (pc) (M) (M) (M pc-2)
1 2.24 ± 0.34 <0.84** <266.8 ± 91.9 9.4 ± 3.6 >4.2 ± 2.3 <28.4 ± 14.7
2 268.56 ± 22.11 0.71 ± 0.10 2414.2 ± 382.2 1128.0 ± 413.4 712.0 ± 297.9 2.1 ± 0.9
3 1.54 ± 0.16 0.13 ± 0.02* 88.0 ± 21.8 6.5 ± 2.4 120.0 ± 53.2 13.6 ± 6.1
4 0.18 ± 0.04 <0.84** <194.8 ± 163.2 0.7 ± 0.3 >0.3 ± 0.3 <262.8 ± 246.5
5 1.34 ± 0.13 <0.84** <1028.6 ± 316.7 5.6 ± 2.1 >2.5 ± 1.3 <182.5 ± 87.8
6 0.84 ± 0.20 0.36 ± 0.11* 457.0 ± 187.9 3.5 ± 1.5 8.7 ± 5.3 129.3 ± 76.8
7 1.03 ± 0.09 <0.84** <1086.5 ± 172.6 4.3 ± 1.6 >1.9 ± 0.8 <251.5 ± 101.0
8 1.78 ± 0.08 <0.84** <714.3 ± 45.4 7.5 ± 2.7 >3.4 ± 1.2 <95.5 ± 34.9
9 0.71 ± 0.10 0.22 ± 0.06* 163.3 ± 56.9 3.0 ± 1.2 19.6 ± 10.5 54.6 ± 28.4
10 6.20 ± 0.57 0.32 ± 0.06* 383.0 ± 87.2 26.0 ± 9.6 81.5 ± 36.3 14.7 ± 6.4
11 7.20 ± 0.59 0.40 ± 0.04* 995.3 ± 144.2 30.3 ± 11.1 60.2 ± 23.9 32.9 ± 13.0
12 10.41 ± 0.82 0.40 ± 0.06* 646.0 ± 115.6 43.7 ± 16.0 86.8 ± 36.0 14.8 ± 6.0
13 3.57 ± 0.30 <0.84** <1186.6 ± 319.3 15.0 ± 5.5 >6.8 ± 3.3 <79.1 ± 36.0
14 4.15 ± 0.41 <0.84** <682.9 ± 191.7 17.5 ± 6.5 >7.9 ± 3.8 <39.1 ± 18.2
15 22.64 ± 1.87 <0.84** <2118.7 ± 375.3 95.1 ± 34.9 >42.9 ± 17.9 <22.3 ± 9.1
16 216.18 ± 4.17 0.48 ± 0.01* 902.6 ± 19.3 908.0 ± 324.7 1259.3 ± 452.0 1.0 ± 0.4
17 101.63 ± 3.43 0.33 ± 0.01* 1171.5 ± 103.4 426.8 ± 153.1 1276.8 ± 462.0 2.7± 1.0
18 66.91 ± 2.76 0.44 ± 0.02* 498.5 ± 37.1 281.0 ± 101.0 463.7 ± 169.8 1.8 ± 0.7
19 1.28 ± 0.15 <0.84** <795.9 ± 280.7 5.4 ± 2.0 >2.4 ± 1.2 <148.0 ± 76.2
20 3.32 ± 0.31 0.33 ± 0.05* 1357.4 ± 297.0 14.0 ± 5.2 40.0 ± 17.3 97.3 ± 41.8
21 1.32 ± 0.12 0.41 ± 0.09* 243.0 ± 74.9 5.6 ± 2.1 10.4 ± 5.0 43.8 ± 21.0
22 107.24 ± 8.92 0.71 ± 0.14 1225.4 ± 253.0 450.4 ± 165.2 282.2 ± 128.7 2.7± 1.1
23 112.54 ± 9.15 0.67 ± 0.12 1578.5 ± 310.5 472.7 ± 173.1 336.6 ± 151.3 3.3 ± 1.4
24 1.29 ± 0.12 <0.84** <1355.9 ± 424.4 5.4 ± 2.0 >2.4 ± 1.2 <250.7 ± 121.3

Notes. The table does not include clump 24 because it includes emission from the sidelobes of other stronger clumps. (*)Minor axis is unresolved. (**)Both axes are unresolved.

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