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Table 2

Molecular clouds in N11 identified in CO(2−1) with CPROPS.

Cloud δRA δDec Velocity Radius Δv LCO(2−1) R2−1/1−0 MCO Mvir†† Mvir/MCO


arcmin km s-1 pc km s-1 102 K km s-1 pc2 103   M

1 7.8 8.3 270 13.2  ±  0.5 7.1  ±  0.3 42  ±  8 0.8  ±  0.2 52.0  ±  10.5 125.2  ±  11.2 2.4  ±  0.5
2a 7.1 –2.1 275  < 5.6 3.9  ±  0.9 4  ±  1 2.7  ±  0.5 1.5  ±  0.4  < 17  < 11.2
3 7.0 –1.2 278 9.4  ±  3.7 4.2  ±  1.3 21  ±  11 1.6  ±  0.3 13.1  ±  6.6 31.0  ±  18.2 2.4  ±  1.8
4 6.8 –0.2 280 8.9  ±  1.0 4.1  ±  0.7 34  ±  10 1.0  ±  0.2 33.5  ±  10.3 27.6  ±  10.9 0.8  ±  0.4
5 3.6 5.3 278 12.8  ±  1.0 5.5  ±  0.5 26  ±  5 1.5  ±  0.3 18.5  ±  3.7 71.6  ±  14.5 3.9  ±  1.1
6a 1.5 4.3 279  < 5.6 4.7  ±  1.0 6  ±  2 2.4  ±  0.5 2.6  ±  1.0  < 25  < 9.5
7 4.2 7.0 283 3.2  ±  0.8 3.6  ±  0.5 7  ±  1 1.5  ±  0.3 5.0  ±  1.0 7.7  ±  2.5 1.6  ±  0.6
8 0.5 4.3 286 4.8  ±  1.1 6.8  ±  0.7 27  ±  6 2.9  ±  0.6 9.7  ±  2.1 41.7  ±  14.0 4.3  ±  1.7
9 2.1 5.2 286 9.2  ±  1.5 5.3  ±  0.8 12  ±  3 1.3  ±  0.3 9.6  ±  2.4 49.1  ±  20.0 5.1  ±  2.5
10 5.7 1.7 280 13.1  ±  1.1 4.5  ±  0.3 22  ±  5 2.4  ±  0.5 9.1  ±  1.8 50.2  ±  8.3 5.5  ±  1.4
11 –8.3 –3.1 269 5.0  ±  1.1 2.8  ±  0.3 5  ±  1 1.1  ±  0.2 4.5  ±  1.0 7.1  ±  2.5 1.6  ±  0.7
12 –6.4 0.4 276 6.2  ±  1.4 3.5  ±  0.4 10  ±  3 0.9  ±  0.2 12.5  ±  3.3 14.1  ±  5.2 1.1  ±  0.5
13 –6.9 –1.0 280 16.0  ±  1.6 5.9  ±  0.8 39  ±  8 1.1  ±  0.2 45.0  ±  9.5 104.2  ±  30.0 2.3  ±  0.8
14 –6.2 –5.6 279 10.4  ±  0.9 5.9  ±  0.5 73  ±  15 0.9  ±  0.2 78.7  ±  16.5 67.7  ±  16.9 0.9  ±  0.3
15 –6.4 –3.9 284 7.5  ±  3.2 4.2  ±  1.1 9  ±  4 0.8  ±  0.2 12.1  ±  5.5 25.2  ±  13.8 2.1  ±  1.5
16 –7.9 –5.7 271 6.8  ±  0.7 4.5  ±  0.4 10  ±  2 0.7  ±  0.1 17.2  ±  3.6 26.2  ±  5.1 1.5  ±  0.4
17 –0.3 –3.9 269 6.1  ±  0.6 4.5  ±  0.6 9  ±  2 0.7  ±  0.1 12.1  ±  2.6 22.8  ±  6.6 1.9  ±  0.7
18 –3.0 –9.1 278 14.4  ±  2.4 2.8  ±  0.5 39  ±  10 0.8  ±  0.2 51.0  ±  12.6 20.7  ±  8.2 0.4  ±  0.2
19 –2.3 –7.9 280 7.7  ±  2.2 2.4  ±  0.5 12  ±  4 1.2  ±  0.2 10.9  ±  3.3 8.4  ±  4.3 0.8  ±  0.5

Notes. Offset positions are relative to , J2000.0. The radii correspond to the geometrical radii for each elliptical cloud. Uncertainties include the error-bars in the CPROPS fitting and 20% error in the luminosity due to calibration.

(a)

Clouds unresolved by CPROPS, we use the beam size as upper limit.

(†)

Molecular masses estimated from the CO(2 − 1) luminosity, scaled to CO(1 − 0) by the R2 − 1/1 − 0 values, using the XCO-factor for the LMC estimated by Hughes et al. (2010) of 4.7 × 1020   cm-2   (K   km   s-1)-1 (see Sect. 5.1).

(††)

Virial masses computed with the formula Mvir = 190   Δv2   R for a spherical cloud with a density profile  ∝ r-1 (MacLaren et al. 1988).

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