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Table A.1

Source list showing the position, the distance, and the evolutionary stage of all high-mass star-forming regions.

Source α δ Galactic l Galactic b Distancea Type 24 μm 70 μm Continuum datab
(J2000.0) (J2000.0) [°] [°] [kpc]
IRDC011.1 18:10:28.4 −19:22:34 11.108 −0.115 3.6 IRDC y y ATLASGAL
IRDC028.1 18:42:50.3 −04:03:20 28.343 0.060 4.8 IRDC y y ATLASGAL
IRDC028.2 18:42:52.1 −03:59:54 28.397 0.080 4.8 IRDC y y ATLASGAL
IRDC048.6 19:21:44.4 +13:49:24 48.657 −0.285 2.5 IRDC n n ATLASGAL
IRDC079.1 20:32:22.0 +40:20:10 79.338 0.341 1.0 IRDC − y SCUBA
IRDC079.3 20:31:57.7 +40:18:26 79.269 0.386 1.0 IRDC − y SCUBA
IRDC18151 18:17:50.3 −12:07:54 18.319 1.792 3.0 IRDC − y Mambo
IRDC18182 18:21:15.0 −14:33:03 16.578 −0.081 3.6 IRDC y y Mambo
IRDC18223 18:25:08.3 −12:45:27 18.605 −0.075 3.7 IRDC y y Mambo
IRDC18306 18:33:32.1 −08:32:28 23.297 0.0550 3.8 IRDC n n Mambo
IRDC18308 18:33:34.3 −08:38:42 23.209 −0.001 4.9 IRDC y y Mambo
IRDC18310 18:33:39.5 −08:21:10 23.478 0.115 5.2 IRDC n n Mambo
IRDC18337 18:36:18.2 −07:41:00 24.374 −0.158 4.0 IRDC y y Mambo
IRDC18385 18:41:17.4 −05:09:56 27.179 −0.104 3.3 IRDC y yc Mambo
IRDC18437 18:46:21.8 −02:12:21 30.390 0.123 (6.2) 7.3d IRDC y y Mambo
IRDC18454.1 18:48:02.1 −01:53:56 30.854 −0.109 (3.5) 6.4e IRDC n n Mambo
IRDC18454.3 18:47:55.8 −01:53:34 30.848 −0.083 6.0 (6.4)f IRDC n n Mambo
IRDC19175 19:19:50.7 +14:01:23 48.617 0.214 1.1 IRDC n n Mambo
IRDC20081 20:10:13.0 +27:28:18 66.145 −3.197 0.7 IRDC − ng Mambo
HMPO18089 18:11:51.6 −17:31:29 12.889 0.489 3.6 HMPO Mambo
HMPO18102 18:13:11.3 −18:00:03 12.623 −0.017 2.7 HMPO Mambo
HMPO18151 18:17:58.1 −12:07:26 18.341 1.768 3.0 HMPO Mambo
HMPO18182 18:21:09.2 −14:31:50 16.585 −0.051 3.9h HMPO Mambo
HMPO18247 18:27:31.7 −11:45:56 19.755 −0.129 6.7 HMPO Mambo
HMPO18264 18:29:14.6 −11:50:22 19.884 −0.535 3.28h HMPO Mambo
HMPO18310 18:33:48.1 −08:23:50 23.455 0.063 5.2 (10.4)i HMPO Mambo
HMPO18488 18:51:25.6 +00:04:07 32.991 0.034 5.4 (8.9)i HMPO Mambo
HMPO18517 18:54:14.4 +04:41:40 37.430 1.517 2.9 HMPO Mambo
HMPO18566 18:59:10.1 +04:12:14 37.554 0.200 6.7 HMPO Mambo
HMPO19217 19:23:58.8 +16:57:44 51.679 0.720 10.5 HMPO Mambo
HMPO19410 19:43:11.0 +23:44:10 59.784 0.066 2.1 HMPO Mambo
HMPO20126 20:14:26.0 +41:13:32 78.122 3.633 1.7 HMPO Mambo
HMPO20216 20:23:23.8 +41:17:40 79.127 2.279 1.7 HMPO Mambo
HMPO20293 20:31:12.9 +40:03:20 78.982 0.352 1.3 (2.0)i HMPO Mambo
HMPO22134 22:15:09.1 +58:49:09 103.876 1.856 2.6 HMPO Mambo
HMPO23033 23:05:25.7 +60:08:08 110.093 −0.067 3.5 HMPO Mambo
HMPO23139 23:16:10.5 +59:55:28 111.256 −0.770 4.8 HMPO Mambo
HMPO23151 23:17:21.0 +59:28:49 111.236 −1.238 5.7 HMPO Mambo
HMPO23545 23:57:06.1 +65:24:48 117.315 3.136 0.8 HMPO Mambo
HMC009.62 18:06:15.2 −20:31:37 9.621 0.193 5.7 HMC ATLASGAL
HMC010.47 18:08:38.2 −19:51:50 10.472 0.027 5.8 HMC ATLASGAL
HMC029.96 18:46:04.0 −02:39:21 29.956 −0.017 7.4 HMC ATLASGAL
HMC031.41 18:47:34.2 −01:12:45 31.412 0.308 7.9 HMC ATLASGAL
HMC034.26 18:53:18.5 +01:14:58 34.257 0.154 4.0 HMC ATLASGAL
HMC045.47 19:14:25.7 +11:09:26 45.466 0.045 6.0 HMC ATLASGAL
HMC075.78 20:21:44.1 +37:26:40 75.783 0.343 4.1 HMC SCUBA
NGC7538B 23:13:45.4 +61:28:11 111.542 0.777 2.65 (5.61)j HMC SCUBA
Orion-KL 05:35:14.4 −05:22:31 208.993 −19.385 0.44 HMC SCUBA
W3IRS5 02:25:40.7 +62:05:52 133.715 1.215 1.8 HMC SCUBA
W3H2O 02:27:04.6 +61:52:25 133.949 1.065 2.0 HMC SCUBA
UCH005.89 18:00:30.4 −24:04:00 5.886 −0.392 2.5 UCHii ATLASGAL
UCH010.10 18:05:13.1 −19:50:35 10.099 0.739 4.4 UCHii ATLASGAL
UCH010.30 18:08:55.8 −20:05:55 10.300 −0.147 6.0 UCHii ATLASGAL
UCH012.21 18:12:39.7 −18:24:20 12.208 −0.102 13.5 UCHii ATLASGAL
UCH013.87 18:14:35.8 −16:45:43 13.872 0.280 4.4 UCHii ATLASGAL
UCH030.54 18:46:59.3 −02:07:24 30.535 0.021 6.1 UCHii ATLASGAL
UCH035.20 19:01:46.4 +01:13:25 35.200 −1.741 3.2 UCHii SCUBA
UCH045.12 19:13:27.8 +10:53:37 45.122 0.132 6.9 UCHii ATLASGAL
UCH045.45 19:14:21.3 +11:09:14 45.454 0.060 6.0 UCHii ATLASGAL

Notes. For the IRDCs we indicate whether or not they show embedded 24 or 70 μm point sources with y(es) or n(o) (or “−” if there are no data available). In the last column the sources of the dust continuum data are presented.

(a)

Unbracketed values are preferred, bracketed values are alternative values.

(b)

Dust continuum data. Either from IRAM 30 m observations with Mambo (1.2 mm), the galactic plane survey ATLASGAL (870 μm; Schuller et al. 2009), or the SCUBA Legacy Catalog (850 μm; Di Francesco et al. 2008).

(c)

Very weak emission compared with the background located at the same position as 24 μm emission source.

(d)

For vlsr = (97.6)111.3 km s-1.

(e)

For vlsr = (52.8)100.2 km s-1.

(f)

For vlsr = 94.3(98.4) km s-1.

(g)

No embedded central point source found, a nearby extended source with emission inside the beam is detected.

(i)

For the near (far) kinematic solution.

(j)

Parallactic (kinematic) distance.

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