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Table H.2.

YSO content of the Galactic giant molecular filaments.

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15) (16) (17) (18)
ID Name Log() Log() Log() Log() Log(SFR) Log(cSFR) Log(ΣSFR) Log() Log(SFE) Log(SFEdense) R Overlap?
GMF (M⊙) (M⊙) (M⊙) (M⊙ Myr−1) (M⊙ Myr−1) (M⊙ Myr−1 pc−2) (M⊙ Myr−1 pc−1)
2 F19 10 20 14 2.23 ± 1.29 2.69 1.73 1.43 2.44 2.19 1.70 0.15 0.95 −1.66 −1.34 0.2 Y
3 GMF20.0−17.9 161 253 201 1.79 ± 0.66 3.49 3.08 2.78 3.24 3.07 3.05 −0.18 0.91 −2.00 −1.70 0.6 Y
6 BC_021.25−0.15 15 21 18 2.20 ± 0.61 2.35 1.94 1.64 2.08 1.92 1.91 −0.38 0.38 −2.05 −0.62 0.3 N
7 G022.519−0.025 56 216 192 2.92 ± 0.58 3.72 2.96 2.66 3.48 3.24 2.93 −0.13 1.36 −1.91 −1.51 0.2 N
8 F21 127 300 248 2.52 ± 0.59 3.84 3.05 2.75 3.59 3.35 3.01 0.13 1.44 −1.74 −1.53 0.3 Y
9 F23 144 337 265 3.03 ± 0.56 3.97 3.27 2.97 3.72 3.49 3.24 0.12 1.60 −1.69 −1.35 0.2 Y
11 F22 81 149 105 2.86 ± 0.60 3.60 2.89 2.58 3.36 3.12 2.85 0.22 1.56 −1.78 −1.65 0.3 Y
12 CFG024.00+0.48 50 113 96 2.35 ± 0.63 3.32 2.77 2.46 3.07 2.87 2.73 −0.27 0.89 −1.99 −1.42 0.4 N
13 F26 24 60 46 2.28 ± 0.61 3.07 2.17 1.87 2.82 2.57 2.14 −0.21 0.91 −2.07 −1.81 0.3 Y
14 F27 47 103 84 3.04 ± 0.59 3.38 2.72 2.42 3.13 2.91 2.69 −0.02 1.16 −1.84 −1.52 0.3 Y
15 BC_24.95−0.17 134 334 282 2.35 ± 0.60 3.78 2.99 2.69 3.53 3.29 2.95 0.14 1.46 −1.62 −1.15 0.3 Y
16 BC_025.24−0.45 44 121 109 2.33 ± 0.61 3.24 2.25 1.95 2.98 2.72 2.22 −0.37 1.03 −2.15 −1.72 0.6 Y
17 F28 19 39 35 1.93 ± 0.68 2.80 2.40 2.10 2.55 2.38 2.37 0.22 0.88 −1.64 −1.39 0.4 Y
18 F29 77 130 105 2.34 ± 0.60 3.45 2.84 2.54 3.20 2.99 2.81 −0.24 1.16 −2.05 −1.70 0.5 Y
19 G025.762+0.241 13 19 13 4.71 ± 1.07 2.98 2.67 2.37 2.73 2.59 2.64 −0.18 0.91 −2.01 −1.75 0.6 N
20 BC_26.94−0.30 7 5 4 2.40 ± 1.80 2.05 1.92 1.62 1.81 1.73 1.89 −0.42 0.30 −2.15 −1.56 3.1 N
21 F30 25 43 36 2.27 ± 0.61 2.91 2.11 1.81 2.66 2.42 2.08 −0.44 0.73 −2.19 −1.65 0.8 N
22 F31 283 715 620 2.01 ± 0.63 4.04 3.16 2.86 3.78 3.53 3.13 0.01 1.49 −1.77 −1.31 0.4 Y
23 CFG028.68−0.28 29 72 61 2.54 ± 0.60 3.12 2.11 1.81 2.87 2.61 2.07 −0.26 0.93 −2.13 −1.92 0.4 Y
24 G028.854−0.238 20 39 33 3.48 ± 0.53 3.07 2.17 1.87 2.82 2.57 2.14 −0.72 0.79 −2.54 −2.19 0.5 Y
25 CFG029.18−0.34 18 64 56 2.94 ± 0.58 3.05 2.07 1.77 2.79 2.53 2.04 −0.55 0.70 −2.47 −2.29 0.7 N
26 G030.315−0.154 101 200 178 2.45 ± 0.60 3.62 2.94 2.63 3.38 3.15 2.90 0.06 1.48 −1.87 −1.70 0.4 Y
27 G32.02+0.06 39 80 65 2.41 ± 0.64 3.28 2.46 2.16 3.04 2.79 2.43 −0.31 0.82 −2.16 −1.88 1.3 N
29 F34 63 69 41 3.12 ± 0.55 3.35 3.25 2.95 3.11 3.04 3.21 −0.28 0.98 −1.98 −1.13 0.3 Y
30 G033.104+0.068 22 13 6 4.16 ± 1.75 2.69 2.48 2.18 2.45 2.34 2.44 −0.89 0.20 −2.57 −1.83 0.4 Y
31 G033.685−0.020 123 130 93 3.22 ± 0.52 3.52 3.33 3.03 3.27 3.17 3.30 −0.43 0.85 −2.21 −1.82 0.4 Y
32 GMF38.1−32.4b 84 144 120 1.64 ± 0.66 3.21 2.39 2.09 2.95 2.71 2.36 −0.06 0.86 −1.76 −1.03 0.4 Y
33 GMF38.1−32.4a 430 677 529 1.96 ± 0.64 3.98 3.23 2.93 3.72 3.49 3.20 −0.29 1.13 −2.06 −1.65 0.8 Y
35 GMF41.0−41.3 34 51 39 1.33 ± 0.61 2.66 2.14 1.84 2.39 2.20 2.11 −0.36 0.49 −1.99 −0.56 0.6 N
37 F39 29 13 6 4.01 ± 0.88 2.65 2.63 2.33 2.41 2.38 2.60 −1.16 0.37 −3.04 −2.84 3.4 N
38 F40 40 32 16 3.40 ± 1.10 2.96 2.35 2.04 2.71 2.50 2.31 −1.05 0.51 −2.79 −2.24 1.3 N
39 CFG047.06+0.26 24 25 21 2.40 ± 0.62 2.49 1.94 1.64 2.23 2.03 1.90 −0.41 0.38 −2.25 −1.95 8.2 N
41 CFG049.21−0.34 65 47 42 2.79 ± 0.60 3.05 2.99 2.69 2.80 2.75 2.95 −0.17 0.66 −2.04 −1.81 0.5 Y
42 F42 118 87 72 2.50 ± 0.60 3.25 2.88 2.58 3.00 2.84 2.84 −0.43 1.04 −2.27 −1.98 0.6 Y
43 GMF54.0−52.0 105 177 146 0.92 ± 0.43 3.11 2.40 2.10 2.85 2.62 2.36 0.28 1.00 −1.52 −1.16 2.7 N
44 GMF307.2−305.4 732 990 922 1.25 ± 0.60 3.89 3.47 3.17 3.63 3.46 3.44 −0.45 1.10 −2.26 −1.90 3.3 N
45 GMF309.5−308.7 296 362 326 1.80 ± 0.65 3.52 3.01 2.71 3.25 3.06 2.98 −0.76 0.98 −2.61 −2.34 1.9 N
46 GMF319.0−318.7 429 498 449 1.40 ± 0.63 3.58 2.99 2.69 3.32 3.11 2.96 −0.53 1.10 −2.39 −2.17 3.5 N
47 GMF324.5−321.4b 51 78 75 0.99 ± 0.47 2.74 2.17 1.86 2.48 2.28 2.13 −0.08 0.77 −1.86 −1.47 17.7 N
48 G322.363+0.542 6 11 8 3.92 ± 1.19 2.72 1.80 1.50 2.48 2.22 1.77 −1.28 0.03 −3.06 −2.66 10.0 N
50 G327.157−0.256 240 340 284 1.74 ± 0.66 3.67 3.48 3.18 3.42 3.32 3.45 −0.20 1.30 −2.00 −1.67 0.7 N
51 GMF335.6−333.6b 301 477 374 1.62 ± 0.66 3.70 3.07 2.77 3.45 3.23 3.04 0.06 1.34 −1.77 −1.48 0.5 N
52 GMF335.6−333.6a 1524 2397 2012 1.80 ± 0.65 4.45 3.91 3.61 4.19 3.99 3.87 −0.16 1.57 −2.10 −1.93 1.6 N
53 Nessie 51 137 98 1.47 ± 0.65 3.18 2.28 1.97 2.92 2.67 2.24 0.23 0.87 −1.52 −1.34 … N
54 GMF341.9−337.1 605 1158 947 1.90 ± 0.65 4.18 3.53 3.22 3.92 3.70 3.49 −0.22 1.52 −2.11 −1.88 1.2 N
57 GMF358.9−357.4 56 97 70 1.85 ± 0.66 2.97 2.18 1.88 2.71 2.47 2.15 −0.27 0.87 −2.09 −1.79 0.9 N

Notes. Columns are: (1) GMF ID; (2) GMF name; (3) number of detected Class I sources; (4) number of detected Class II sources; (5) number of Class II sources with the Ks band detection; (6) mass completeness of Class II sources; (7) total number of Class II sources estimated assuming a universal IMF; (8) total number of Class I sources estimated assuming a universal luminosity function; (9) total mass of Class I sources; (10) total mass of Class II sources; (11) star formation rate; (12) current star formation rate obtained with only Class I sources; (13) surface density of star formation rate; (14) star formation rate per unit length; (15) star formation efficiency; (16) dense gas star formation efficiency; (17) 13CO flux ratio of GMF to other velocity components. High value implies that the GMF is the dominating component along the line of sight; (18) overlap with other GMFs? We note that the associated uncertainties of the parameters listed in this table do not include the distance errors (also see Appendix D for more information).

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