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Table A.1.

Properties of the molecular clouds identified in the 12CO (1–0) data cubes.

Index Name l b ma mi PA vLSR σv ICO LCO d
(°) (°) (″) (″) (°) (km s−1) (km s−1) (K km s−1) (K km s−1 pc2) (kpc)
1 FQS-MC219.856-2.190 219.8564 −2.1897 74.24 22.85 84.01 28.49 0.80 10.712 13.97 2.332
3 FQS-MC219.921-2.098 219.9211 −2.0981 75.33 42.80 52.40 31.76 1.00 8.437 26.20 2.649
4 FQS-MC220.030-1.363 220.0299 −1.3631 74.14 45.43 113.61 17.23 0.70 5.851 3.71 1.319
7 FQS-MC220.158-1.482 220.1583 −1.4822 119.40 31.85 55.38 70.09 1.01 22.190 229.31 7.896

R A M Σ αvir nl flag1 flag2

(pc) (pc2) (M) (M pc−2)
0.889 2.30 0.00 0.00 0.00 1 1 2
1.393 4.91 18.37 3.74 88.34 1 1 0
0.709 0.98 44.49 45.27 9.06 1 0 2
4.509 52.83 2888.87 54.68 1.86 1 0 0

Notes. Columns are as follow: Col. 1: progressive index. Column 2: name defined as “FQS-MC” followed by the Galactic coordinates of the cloud’s centroid. Columns 3 and 4: Galactic longitude and latitude of the cloud’s centroid. Columns 5 and 6: intensity-weighted semi-major and semi-minor axes, ma and mi, respectively. Column 7: position angle with respect to the cube x-axis. Column 8: mean velocity. Column 9: velocity dispersion. Column 10: 12CO (1–0) integrated intensity across the area of the cloud. Column 11: total luminosity from the 12CO (1–0) line. Column 12: kinematic distance from the Sun. Column 13: equivalent radius, assuming circular geometry. Column 14: area. Column 15: total mass derived from Herschel H2 column density. Column 16: average surface density. Column 17: virial parameter. Column 18: number of dendrogram leaves. Column 19: flag1; 0 indicates that the cloud is fully mapped in the Herschel H2 column density map, 1 indicates that the area of the cloud as derived from the 12CO (1–0) data is only partially covered, or not covered at all, by the Herschel H2 column density map; for those clouds the derived mass and surface density are lower limits and the virial parameter is an upper limit. Column 20: flag2; 0 means that the cloud is fully mapped in 12CO (1–0), 2 means that the area of the cloud as derived from the 12CO (1–0) touches the border of the map; those clouds could extend outside the mapped area, therefore the measured parameters are linked to an uncertainty that depends on how much CO emission was missed. Only a few objects are listed as example here, the complete catalogue is available at CDS.

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