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Table D.1.

Fit parameters and virial masses of sources with a peaked emission in 12CO, 13CO or C18O.

ID Comp. VLSR σ12 σ13 σ18 N13 N18 M13 M18 Mdust Evol.
[km s−1] [K] [K] [K] [km s−1] [km s−1] [km s−1] [cm−2] [cm−2] [M] [M] [M] [M] [M]
1446 1 8.27 16.44 7.12 0.98 1.00 0.60 0.50 1.7e+16 1.7e+15 19.4 13.7 7.8 6.3 21.6 0.9 0.6 4
2 10.00 4.00 0.39 0.10 4.00 1.02 0.60 1.0e+15 1.5e+14 56.0 19.7 0.4 0.5 21.6 2.6 0.9 4
1448 1 7.86 12.27 8.45 1.22 0.94 0.55 0.48 2.0e+16 1.8e+15 12.3 9.4 7.2 5.4 15.3 0.8 0.6 4
1449 1 7.56 14.15 8.36 1.51 0.51 0.47 0.36 1.6e+16 1.8e+15 11.3 6.5 7.0 6.1 23.0 0.5 0.3 4
1450 1 5.81 12.97 6.21 0.89 1.80 0.85 0.62 2.0e+16 1.7e+15 53.2 28.3 11.8 8.4 51.7 1.0 0.5 0
2 7.44 11.02 8.11 1.34 0.95 0.48 0.41 1.6e+16 1.6e+15 16.7 12.1 9.6 7.9 51.7 0.3 0.2 0
1451 1 5.94 16.50 8.25 1.57 0.66 0.65 0.54 2.3e+16 3.0e+15 25.8 18.1 11.4 12.3 16.3 1.6 1.1 3
2 7.57 23.32 10.69 1.06 0.64 0.46 0.40 2.5e+16 1.8e+15 12.9 9.8 12.5 7.4 16.3 0.8 0.6 3
1453 1 8.53 17.33 8.15 1.81 0.70 0.43 0.32 1.5e+16 2.1e+15 10.3 5.5 6.8 7.7 22.3 0.5 0.2 2
1454 1 5.29 9.41 6.74 2.71 1.13 0.51 0.34 1.3e+16 2.8e+15 17.7 8.0 7.4 12.7 32.0 0.6 0.2 4
1459 1 7.71 18.38 10.58 1.91 1.02 0.48 0.31 2.4e+16 2.2e+15 11.2 4.8 9.9 7.6 4.4 2.5 1.1 1
1460 1 5.81 5.31 1.44 0.06 0.46 0.56 1.42 2.2e+15 2.0e+14 15.3 98.9 0.9 0.7 8.5 1.8 11.6 2
2 7.99 15.00 8.56 3.30 1.25 0.49 0.22 1.8e+16 2.6e+15 11.8 2.4 7.3 8.7 8.5 1.4 0.3 2
1461 1 4.98 5.77 2.64 0.67 0.22 0.22 0.33 1.7e+15 5.6e+14 4.1 9.4 1.3 3.4 13.3 0.3 0.7 2
2 5.65 12.35 5.66 2.08 0.59 0.59 0.36 1.2e+16 2.4e+15 30.5 11.2 8.9 14.2 13.3 2.3 0.8 2
1463 1 5.47 12.93 6.07 1.76 0.45 0.45 0.32 1.0e+16 1.8e+15 8.7 4.6 3.9 5.7 4.7 1.9 1.0 2
1464 1 5.92 9.29 5.70 0.92 0.87 0.82 0.54 1.7e+16 1.4e+15 34.3 14.8 7.2 4.8 2.9 11.8 5.1 1
2 8.45 17.48 6.64 0.81 0.72 0.36 0.24 9.7e+15 6.9e+14 6.6 3.0 4.2 2.4 2.9 2.3 1.0 1
1469 1 5.43 7.04 5.27 2.47 2.03 0.49 0.26 9.6e+15 1.9e+15 16.9 5.0 5.6 8.9 13.7 1.2 0.4 2
1470 1 8.28 18.92 8.88 1.08 0.95 0.43 0.31 1.7e+16 1.3e+15 9.9 5.1 7.6 4.5 2.8 3.5 1.8 1
1471 1 7.31 6.38 5.67 0.96 1.70 0.31 0.14 7.6e+15 3.6e+14 4.8 1.0 3.2 1.2 2.9 1.7 0.3 4
1472 1 6.82 16.57 8.64 1.45 1.29 0.70 0.49 2.6e+16 2.5e+15 26.1 13.0 11.5 9.1 8.5 3.1 1.5 1
1477 1 5.21 4.23 2.14 0.96 0.45 0.45 0.26 2.9e+15 6.6e+14 17.7 5.9 2.2 4.0 2.2 8.0 2.7 2
1480 1 8.14 15.21 8.63 2.11 1.38 0.59 0.30 2.1e+16 2.2e+15 12.8 3.3 7.6 6.2 2.8 4.6 1.2 2
1484 1 5.87 10.85 4.39 0.79 0.89 0.57 0.26 8.3e+15 6.0e+14 14.4 3.1 3.3 1.9 2.2 6.5 1.4 0
1486 1 7.85 16.64 7.87 0.69 0.71 0.41 0.35 1.4e+16 8.4e+14 10.5 7.6 6.9 3.5 1.2 8.8 6.3 2
1491 1 9.13 16.24 3.10 0.10 0.62 0.39 0.25 4.4e+15 8.0e+13 11.0 4.4 2.6 0.4 2.4 4.6 1.8 2
1495 1 6.49 9.75 4.99 0.83 1.03 0.75 0.48 1.3e+16 1.1e+15 36.0 15.0 6.7 4.8 1.5 24.0 10.0 2
2 9.12 15.39 6.38 0.53 0.79 0.43 0.34 1.1e+16 6.0e+14 11.8 7.6 5.6 2.6 1.5 7.9 5.1 2
1514 1 6.55 7.11 5.48 0.90 2.08 0.54 0.27 1.1e+16 6.5e+14 14.3 3.7 4.7 2.2 1.2 11.9 3.1 2
2 8.82 11.62 7.25 0.83 0.72 0.46 0.34 1.3e+16 8.5e+14 10.6 5.9 5.5 2.9 1.2 8.8 4.9 2
1518 1 5.40 11.10 7.42 1.58 1.13 0.56 0.39 1.6e+16 1.9e+15 14.9 7.3 6.7 6.2 1.6 9.3 4.6 2
1521 1 5.74 9.58 3.39 0.36 1.27 0.57 0.28 6.0e+15 2.8e+14 23.1 5.5 3.5 1.3 1.4 16.5 3.9 2
2 8.76 16.70 7.39 0.56 0.50 0.35 0.32 1.1e+16 6.3e+14 9.0 7.5 6.3 3.0 1.4 6.4 5.4 2
1528 1 5.49 14.71 3.92 0.28 0.63 0.41 0.26 5.7e+15 2.3e+14 9.5 3.8 2.6 0.9 0.6 15.8 6.3 2
2 5.41 0.12 1.73 0.18 0.37 0.15 0.03 6.6e+15 2.3e+14 - - 3.3 1.0 0.6 2

Notes. The columns are (1) the index of the source in the GCC catalogue; (2) the index of the velocity component; (3) the centroid velocity of the velocity component; (4–6) the peak Tmb of the Gaussian fit to the current velocity component of the 12CO, 13CO, and C18O lines; (7–9) the standard deviation of the Gaussian fit to the current velocity component of the 12CO, 13CO, and C18O lines; (10–11) Column density of 13CO and C18O; (12–13) Virial mass from 13CO and C18O line widths; (14–15) Core mass from 13CO and C18O; (16) Estimates of the core mass from the GCC catalogue; (17–18) the virial parameters from 13CO and C18O (1-0) lines; and(19) the new estimate of the evolutionary stage of the source. The code is: 0 = undetermined, 1 = candidate starless core, 2 = reliable starless core, 3 = candidate protostellar core, 4 = confirmed protostellar core. ( ⋆ )This component corresponds to the non-Gaussian shape of the first component peak, hence the very low value of . The quantities marked with † were derived from a full integration of the line profile, therefore including both components.

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