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Table 3

Core properties, method comparison.

IRDC ID Notes
No. a (M) (M) (M) (K) (K) (L) (L)

IRDC 310.39–0.30
1d 303 229 (2054) 246 (391) 17 18 (16) 716 660 (793)

IRDC 316.72+0.07
6 9 3 (30) 4 (81) 17 18 (12) 19 14 (32)
7 93 (462) 93 (659) 12 (10) 31 (78)
8 6 2 (17) 2 (44) 20 22 (14) 34 31 (55)
9 8 8 (36) 9 (64) 18 17 (13) 26 25 (42)
16 1 1 (5) 1 (8) 20 19 (14) 5 9 (12)
18 14 12 14 7
19 22 (50) 26 (70) 12 (11) 9 (14)
22d 7 25 (177) 18 (72) 16 15 (13) 12 19 (38)
24 8 (25) 10 (40) 15 (13) 11 (17)
25 2 (10) 2 (10) 19 (14) 10 (16)
29 12 8 8 16 16 16 14
32 22 7 9 14 15 16 10
35 13 23 24 19 17 54 63
36 16 7 10 16 16 21 17
38 79 90 (228) 86 (201) 25 25 (21) 1650 1672 (1972)
42 17 15 14 11

IRDC 320.27+0.29
3 2 (7) 2 (11) 16 (13) 3 (5)
4 5 3 (10) 3 (14) 18 18 (15) 14 13 (20)

IRDC 321.73+0.05
2 3 34 28 22 15 32 62
3 1 2 1 23 22 16 21
4 24 43 36 18 17 71 84
5 4 9 8 18 16 12 15

IRDC 009.86–0.04
2 2 3 2 24 22 37 70

IRDC 011.11–0.12
4 5 36 30 23 17 68 119
7 25 10 (35) 13 (55) 20 22 (17) 152 142 (197)
14 2 17 14 21 15 16 27
17 4 6 5 23 21 51 72
18 80 183 (302) 169 (365) 24 21 (17) 1444 1857 (2064)
24 3 1 (5) 1 (10) 22 26 (17) 32 32 (47)
27 116 75 12 21
28 6 (23) 7 (34) 18 (15) 24 (34)
33 4 3 3 24 24 73 80

IRDC 18223
2 10 17 (44) 17 (62) 21 19 (15) 79 104 (130)
3 9 25 23 20 17 51 62
4 61 143 (240) 122 (324) 20 18 (15) 323 383 (436)
6 12 99 (211) 86 (292) 24 17 (13) 200 349 (407)
7 185 254 (450) 256 (548) 22 21 (18) 1979 4814 (5154) IRAS 18223-1243
8 51 2 (15) 4 (31) 18 24 (18) 156 81 (132)
9 3 4 20 22
10 7 14 14 20 17 33 41

IRDC 019.30+0.07
1 12 13 13 18 17 33 34
2 0.8 4 3 25 19 19 33
3 37 36 38 20 20 219 229

IRDC 028.34+0.06
2 93 782 (1062) 671 (1132) 28 18 (16) 3577 8058 (8470) MSX G028.3373+00.1189
4 22 (67) 20 (80) 17 (15) 50 (71)
7 14 37 34 20 17 85 106
8 49 1369 971 18 12 151 357
9d 534 4490 (9249) 3496 (6720) 20 15 (14) 2950 4703 (5488) MSX G028.3937+00.0757
11 265 110 (286) 140 (332) 14 15 (13) 177 134 (201)
15 9 5 (18) 6 (25) 20 21 (16) 52 48 (66)
18 19 (71) 17 (87) 17 (14) 41 (64)

Notes.

(a)

From Table B.1;

(c)

derived with the best fit dust temperature (Col. 6 of this table);

(d)

leaf overlaps with multiple Herschel cores. SABOCA flux is scaled according to luminosity ratio of cores (see Sect. 3.2).

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