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Table 4

Physical properties derived for the ten CHIMPS 13CO (3–2) clumps with the greatest integrated emission.

Designation KDA Method dk RGC M Rσ Req αvir PthermkB PturbkB
[kpc] [kpc] [103M] [pc] [pc] [103 cm−3] [K] [104 K cm−3] [106 K cm−3]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
G043.167+00.017 F iii 11.96 8.19 135 3.55 9.16 0.62 0.86 22.1 1.4 14.3
G034.238+00.115 N iii 3.43 5.83 13 1.19 2.76 2.22 0.58 14.7 3.3 10.2
G034.248+00.166 N iii 3.38 5.86 19 1.42 3.18 2.10 0.51 12.7 2.7 10.1
G043.163-00.031 F iii 11.37 7.78 56 3.15 7.66 0.44 1.18 18.4 0.8 6.5
G029.910-00.059 N iii 6.25 4.27 10 1.78 4.12 0.49 2.09 20.5 1.0 4.0
G030.838-00.059 N iii 5.91 4.45 8 1.77 4.21 0.40 3.35 17.3 0.7 4.5
G030.722-00.098 N viii 5.21 4.69 19 1.64 3.93 1.10 1.56 14.0 1.5 14.0
G029.961-00.015 N iii 5.83 4.39 8 1.53 3.49 0.69 1.64 20.5 1.4 4.4
G030.437-00.235 N iii 6.45 4.29 9 2.30 5.44 0.19 1.41 17.1 0.3 0.7
G029.860-00.050 N iii 6.05 4.32 7 1.59 3.75 0.48 1.78 21.2 1.0 2.8

Notes.The columns detail the following: (1) source designation; (2) kinematic-distance-ambiguity (KDA) solutions, where near, tangential and far kinematic distances are designated by “N”, “T” and “F”, respectively; (3) method used to resolve the KDA; (4) heliocentric distance; (5) Galactocentric distance; (6) mass of H2; (7) intensity-weighted rms radius; (8) equivalent radius; (9) volume-averaged particle density; (10) virial parameter; (11) mean voxel excitation temperature; (12) thermal pressure; and (13) isotropic turbulent pressure. Only a portion of the full table is shown here to illustrate its form and content. The full table can be downloaded in a machine-readable format fromthe CANFAR archive and is available at the CDS.

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