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Table 1

Properties of the IRDCs.

#a l b D b σ v σ v σ v σ v σ N/⟨N Σsatc M MIR M combined α vir
(G, box)d (F, box)d (G, ell)d (F, ell)d (box)d
[°] [°] [kpc] [km s-1] [km s-1] [km s-1] [km s-1] [g cm-2] [103 M] [103 M]

A 18.822 –0.285 4.8 2.04 3.44 2.05 3.78 0.63 0.496 17.7 18.5 1.4
B 19.271 0.074 2.4 1.60 1.71 1.77 1.79 0.69 0.488 2.2 2.2 2.2
C 28.373 0.076 5.0 3.72 3.38 3.75 3.41 0.80 0.520 45 53.2 2.4
D 28.531 –0.251 5.7 1.85 2.12 2.01 2.14 0.67 0.436 53.4 74.3e 0.5
E 28.677 0.132 5.1 4.32 1.94 2.15 2.55 0.60 0.504 25.2 28.7 1.1
F 34.437 0.245 1.56f 3.62 4.15 1.86 2.54 0.73 0.370 0.79f 0.85 3.5
G 34.771 –0.557 2.9 3.28 3.15 2.95 2.90 0.57 0.347 2.01 3.3 4.7
H 35.395 –0.336 2.9 2.03 2.11 1.48 1.78 0.52 0.416 13.34 16.7 0.7
I 38.952 –0.475 2.7 1.65 1.72 1.26 1.32 0.63 0.402 2.05 2.7 1.2
J 53.116 0.054 1.8 0.96 1.14 0.83 0.95 0.50 0.328 0.08 0.2 1.5

Notes. 

(a)

Naming according to BT09.

(c)

Saturation limit, i.e., the maximum observable mass surface density, of the mid-infrared data (cf., BT12).

(d)

The letters G(aussian) and F(ixed range) refer to the two approaches used in estimating the velocity dispersions in the clouds (see Sect. 2.4). The abbreviations box and ell refer to the two approaches used in defining the cloud area (see Sect. 3.2).

(e)

Mcombined can be somewhat underestimated because of incomplete coverage of the NIR data, see Fig. B.4.

(f)

The distance for the cloud F has been recently derived from parallax measurements (Kurayama et al. 2011) and we adopt this distance (however, see also Foster et al. 2012). For comparison, the GRS distance for the cloud is D = 3.7 kpc).

(g)

The mass given by BT12 was scaled to correspond the adopted distance.

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