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Table A.2

Properties of the Hi-GAL sources toward G345.5+1.5.

Id ℓ b T Menv Lbol Lsub /Lbol IR Id ℓ b T Menv Lbol Lsub/Lbol IR
° (K) M⊙ L⊙ (%) ° (K) M⊙ L⊙ (%)
1 344.813 1.250 17.1 ± 1.3 4 ± 1 11 ± 7 4.1 Prestellar 41 345.193 1.030 28.7 ± 0.9 306 ± 19 2245 ± 541 2.8 Protostellar
2 344.865 1.190 10.3 ± 0.5 80 ± 23 9 ± 5 22.4 Prestellar 42 345.194 1.052 20.5 ± 1.7 22 ± 7 188 ± 148 1.7 Protostellar
3 344.900 1.204 8.7 ± 0.4 268 ± 111 11 ± 7 35.8 Prestellar 43 345.197 0.980 15.2 ± 1.2 38 ± 31 358 ± 449 0.8 Protostellar
4 344.901 1.227 14.0 ± 1.3 16 ± 7 12 ± 11 8.7 Prestellar 44 345.198 1.150 21.5 ± 1.9 6 ± 2 77 ± 60 1.4 Protostellar
5 344.912 1.178 13.8 ± 0.9 28 ± 7 16 ± 10 10.1 Prestellar 45 345.199 0.863 15.4 ± 1.5 7 ± 6 9 ± 13 6.1 Prestellar
6 344.924 1.093 12.6 ± 0.5 39 ± 31 15 ± 16 12.2 Prestellar 46 345.209 1.015 27.7 ± 1.9 17 ± 14 619 ± 759 0.7 Protostellar
7 344.931 1.213 11.3 ± 0.7 56 ± 19 11 ± 8 17.4 Prestellar 47 345.211 1.051 16.5 ± 1.9 139 ± 53 229 ± 248 5.6 Prestellar
8 344.952 1.100 14.4 ± 1.3 37 ± 10 31 ± 26 7.8 Prestellar 48 345.215 1.029 29.2 ± 2.2 84 ± 22 2315 ± 1683 1.0 Protostellar
9 344.952 1.209 14.9 ± 1.3 44 ± 16 43 ± 38 7.4 Prestellar 49 345.216 0.946 14.8 ± 1.0 20 ± 16 32 ± 40 4.4 Protostellar
10 344.954 1.005 11.6 ± 0.6 47 ± 38 11 ± 12 15.7 Prestellar 50 345.216 1.019 18.7 ± 1.8 177 ± 87 2196 ± 2352 1.0 Protostellar
11 344.954 1.080 10.7 ± 0.5 56 ± 16 8 ± 4 21.1 Prestellar 51 345.227 0.873 13.9 ± 1.3 10 ± 8 7 ± 10 8.9 Prestellar
12 344.957 1.171 12.9 ± 0.8 129 ± 42 52 ± 36 12.2 Prestellar 52 345.238 1.046 13.7 ± 0.5 307 ± 37 161 ± 58 10.9 Prestellar
13 344.960 1.195 14.3 ± 0.7 98 ± 21 123 ± 63 5.2 Protostellar 53 345.243 1.025 17.0 ± 0.2 115 ± 3 244 ± 21 4.6 Protostellar
14 344.964 1.046 15.2 ± 0.7 15 ± 12 18 ± 19 6.5 Prestellar 54 345.250 1.038 14.9 ± 0.6 113 ± 20 116 ± 48 6.6 Protostellar
15 344.970 0.984 14.8 ± 1.5 17 ± 14 17 ± 24 7.0 Prestellar 55 345.254 1.173 15.4 ± 1.2 16 ± 5 37 ± 28 3.3 Protostellar
16 344.986 1.105 11.1 ± 0.4 88 ± 14 24 ± 9 11.7 Protostellar 56 345.254 1.016 25.1 ± 2.5 9 ± 7 121 ± 166 1.6 Protostellar
17 344.990 0.905 14.2 ± 1.0 8 ± 6 6 ± 7 8.3 Prestellar 57 345.256 1.077 15.4 ± 0.4 133 ± 16 336 ± 95 3.0 Protostellar
18 344.995 1.146 11.1 ± 0.5 115 ± 31 21 ± 11 18.1 Prestellar 58 345.259 1.112 17.1 ± 1.3 33 ± 10 124 ± 92 2.7 Protostellar
19 345.008 1.026 10.8 ± 0.7 89 ± 30 13 ± 10 20.3 Prestellar 59 345.278 1.115 15.0 ± 0.8 39 ± 9 45 ± 25 6.3 Protostellar
20 345.016 1.210 18.6 ± 1.4 10 ± 2 41 ± 28 2.8 Protostellar 60 345.280 1.079 30.6 ± 2.8 5 ± 4 159 ± 213 1.0 Protostellar
21 345.018 1.160 18.3 ± 1.8 9 ± 3 63 ± 57 1.6 Protostellar 61 345.285 0.931 16.8 ± 0.7 23 ± 19 280 ± 295 0.8 Protostellar
22 345.019 1.027 11.7 ± 0.7 58 ± 47 14 ± 17 15.3 Prestellar 62 345.301 1.039 16.0 ± 0.5 180 ± 19 675 ± 208 2.3 Protostellar
23 345.020 1.065 16.9 ± 0.2 13 ± 10 31 ± 26 4.1 Protostellar 63 345.304 1.071 17.2 ± 2.1 30 ± 25 101 ± 157 3.0 Protostellar
24 345.026 1.090 11.8 ± 0.7 68 ± 24 39 ± 27 6.7 Protostellar 64 345.320 0.913 15.3 ± 1.0 12 ± 10 15 ± 17 6.4 Prestellar
25 345.029 1.135 18.4 ± 1.3 10 ± 2 60 ± 40 2.0 Protostellar 65 345.320 1.141 18.8 ± 2.1 13 ± 4 54 ± 55 3.0 Prestellar
26 345.038 1.014 12.2 ± 0.2 27 ± 20 22 ± 19 5.1 Protostellar 66 345.333 1.101 11.0 ± 0.6 63 ± 20 10 ± 7 19.3 Prestellar
27 345.040 1.104 12.2 ± 1.1 77 ± 33 40 ± 39 8.3 Protostellar 67 345.334 1.021 16.0 ± 0.3 619 ± 53 1338 ± 265 3.6 Protostellar
28 345.047 0.921 20.4 ± 1.8 3 ± 2 17 ± 23 2.4 Protostellar 68 345.336 1.040 10.3 ± 0.4 290 ± 44 52 ± 19 13.3 Protostellar
29 345.055 1.179 15.7 ± 1.1 25 ± 6 36 ± 23 5.7 Prestellar 69 345.343 0.986 18.1 ± 1.8 7 ± 5 22 ± 32 3.6 Prestellar
30 345.057 1.077 16.4 ± 1.3 24 ± 19 116 ± 149 1.8 Protostellar 70 345.346 1.040 13.7 ± 0.5 113 ± 19 55 ± 21 11.5 Prestellar
31 345.069 1.142 18.4 ± 1.6 15 ± 7 55 ± 57 3.2 Prestellar 71 345.362 1.066 22.1 ± 1.9 7 ± 6 180 ± 234 0.7 Protostellar
32 345.079 0.894 11.9 ± 1.0 37 ± 30 10 ± 14 14.6 Prestellar 72 345.362 1.022 17.3 ± 1.9 35 ± 17 85 ± 98 4.3 Prestellar
33 345.090 1.011 16.5 ± 1.6 12 ± 10 71 ± 100 1.5 Protostellar 73 345.367 1.040 15.9 ± 0.5 120 ± 15 163 ± 54 6.2 Prestellar
34 345.097 1.039 13.3 ± 1.0 17 ± 5 8 ± 6 11.2 Prestellar 74 345.374 1.081 30.9 ± 3.3 5 ± 4 133 ± 186 1.2 Protostellar
35 345.106 0.925 15.1 ± 1.1 21 ± 17 41 ± 51 3.9 Protostellar 75 345.379 1.042 15.8 ± 0.9 110 ± 86 163 ± 184 5.6 Prestellar
36 345.114 1.121 14.6 ± 1.3 15 ± 8 41 ± 45 2.5 Protostellar 76 345.383 1.057 11.7 ± 0.5 501 ± 115 1441 ± 685 1.3 Protostellar
37 345.118 0.943 17.8 ± 1.7 6 ± 5 23 ± 31 2.9 Protostellar 77 345.400 1.050 17.6 ± 1.3 9 ± 3 31 ± 23 3.1 Protostellar
38 345.124 1.054 13.8 ± 0.9 25 ± 20 17 ± 20 9.2 Prestellar 78 345.412 1.045 14.1 ± 0.8 39 ± 13 27 ± 18 8.9 Prestellar
39 345.136 1.071 10.7 ± 0.5 387 ± 84 89 ± 43 12.4 Protostellar 79 345.426 1.057 10.1 ± 0.5 154 ± 45 15 ± 9 24.5 Prestellar
40 345.180 1.045 16.6 ± 0.4 524 ± 30 491 ± 4 8.6 Protostellar

Notes. Source id (Col. 1), galactic coordinates (Cols. 2 and 3), envelope temperature (Col. 4), envelope mass (Col. 5), bolometric luminosity (Col. 6), submillimetric to bolometric luminosity ratio (Col. 7), nature of the source (pre/protostellar, Col. 8).

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