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Table A.1

Properties of the clumps derived from modified black body fits to their SEDs.

Source T dust M L bol
(K) (M) (L)

05358+3543 76 70 4370
G213.61-12.6* 39 800 113 000
G189.78+0.34* 42 63 8630
G192.60–0.05* 72 100 60 200
18151-1208_1* 75 120 11 800
G18.15–0.28 105 43 33 400
G18.18–0.30 32 55 2640
18223–1243 73 230 16 100
18228–1312 95 240 29 800
G19.27+0.1M2 29 57 1450
G19.27+0.1M1 33 47 2760
18232–1154 53 61 19 800
18236–1205 60 320 3370
G19.61–0.24A* 59 765 264 000
G20.08–0.1 66 410 19 700
18264–1152 59 440 5970
G23.60+0.0M1 21.5 660 3370
18316–0602 48 610 171 000
G23.60+0.0M2 26 58 1780
18317–0513 79 270 16 200
G24.08+0.0M2* 31 93 2930
G24.33+0.1M1 56 460 17 600
G24.33+0.1M4* 41 460 4890
G24.33+0.1M2* 28 400 7190
G24.60+0.1M2 21 390 2420
G24.60+0.1M1 22 140 772
G25.04–0.2M1 20 350 1320
G25.04–0.2M4* 33 210 869
G25.04–0.2M2* 25 100 1060
G28.28–0.35 109 97 45 100
G34.43+0.2M1 42 380 32 700
18507+0121 61 820 17 700
G34.43+0.2M3 35 95 6940
G34.24+0.13 48 51 31 700
18517+0437* 43 400 27 600
19035+0641* 74 46 5830
19095+0930 61 260 52 100
G43.89–0.38* 57 88 53 100
G61.48+0.09A* 66 189 117 000
20216+4107* 72 17 3180
20332+4124 79 180 23 900
22134+5834* 82 55 12 600
22570+5912_1* 82 180 48 400
23033+5951 71* 170 12 500
NGC7538B* 37 6480 200 000
23139+5939* 71 200 24 100
23151+5912* 98 180 121 000

Notes. 

(*)

Sources whose derived luminosities are upper limits (see Sect. 5.1).

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