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Table A.2.

Example catalog of GMC properties of IC 342.

Cloud RA Dec vLSR R PA e σv MCO Mvir
(J2000) (J2000) (km s−1) (pc) (°) (km s−1) (106 M) (106 M)
1 56.57360 68.029582 -55.7 59 6.8 0.4
2 56.57038 68.033543 -56.1 106.9 8 0.88 7.5 2.6 10.2
3 56.49006 68.052340 -49.2 66.8 174 0.42 6.7 1.2 5.0
4 56.55737 68.010278 -51.2 91.3 147 0.38 5.8 2.2 5.2
5 56.56855 68.011551 -51.7 62.4 22 0.82 4.8 1.2 2.4
6 56.56769 68.017141 -53.3 112.6 20 0.72 7.0 1.2 9.4
7 56.52838 68.030475 -59.5 87.0 24 0.85 11.3 1.3 18.6
8 56.51868 68.031299 -62.6 34 6.8 0.3
9 56.54947 68.024618 -55.2 124.7 44 0.91 3.7 1.7 2.9
10 56.54147 68.030874 -51.6 105.8 125 0.58 8.3 3.2 12.4

Notes. The columns correspond to the cloud coordinates, velocity centroid, deconvolved cloud radius, position angle of the cloud major axis, cloud eccentricity, line width, and cloud luminous and virial mass. The cloud eccentricity is calculated as . MCO is obtained as the cloud CO luminosity (flux in K km s−1 pc2) multiplied by our assumed Galactic CO-to-H2 conversion factor. The virial mass is estimated as . The full table is available at the CDS.

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