Table A.1
List of the observed sources.
| Source | RA(J2000) | Dec(J2000) | VLSR | d | Lbol | Ref. |
| h m s | ° ′ ′′ | km s-1 | kpc | L⊙ | ||
|
|
||||||
| HMSC | ||||||
|
|
||||||
| I00117-MM2a | 00:14:26.3 | +64:28:28 | −36.3 | 1.8 | 103.1 | (1) |
| AFGL5142-ECbw | 05:30:48.7 | +33:47:53 | −3.9 | 1.8 | 103.6 | (2) |
| 05358-mm3bw | 05:39:12.5 | +35:45:55 | −17.6 | 1.8 | 103.8 | (3, 11) |
| G034-G2(MM2)a | 18:56:50.0 | +01:23:08 | + 43.6 | 2.9 | 101.6r | (4) |
| G034-F1(MM8)a | 18:53:19.1 | +01:26:53 | + 57.7 | 3.7 | 101.9r | (4) |
| G034-F2(MM7)a | 18:53:16.5 | +01:26:10 | + 57.7 | 3.7 | – | (4) |
| G028-C1(MM9)a | 18:42:46.9 | −04:04:08 | + 78.3 | 5.0 | – | (4) |
| I20293-WCa | 20:31:10.7 | +40:03:28 | + 6.3 | 2.0 | 103.6 | (5, 6) |
| I22134-Gbw | 22:15:10.5 | +58:48:59 | −18.3 | 2.6 | 104.1 | (7) |
| I22134-Bb | 22:15:05.8 | +58:48:59 | −18.3 | 2.6 | 104.1 | (7) |
|
|
||||||
| HMPO | ||||||
|
|
||||||
| I00117-MM1a | 00:14:26.1 | +64:28:44 | −36.3 | 1.8 | 103.1 | (1) |
| I04579-VLA1c | 05:01:39.9 | +47:07:21 | −17.0 | 2.5 | 103.6 | (8) |
| AFGL5142-MMb | 05:30:48.0 | +33:47:54 | −3.9 | 1.8 | 103.6 | (2) |
| 05358-mm1b | 05:39:13.1 | +35:45:51 | −17.6 | 1.8 | 103.8 | (3) |
| 18089–1732b | 18:11:51.4 | −17:31:28 | + 32.7 | 3.6 | 104.5 | (9) |
| 18517+0437b | 18:54:14.2 | +04:41:41 | + 43.7 | 2.9 | 104.1 | (10) |
| G75-corea | 20:21:44.0 | +37:26:38 | + 0.2 | 3.8 | 104.8 | (11, 12) |
| I20293-MM1a | 20:31:12.8 | +40:03:23 | + 6.3 | 2.0 | 103.6 | (5) |
| I21307a | 21:32:30.6 | +51:02:16 | −46.7 | 3.2 | 103.6 | (13) |
| I23385a | 23:40:54.5 | +61:10:28 | −50.5 | 4.9 | 104.2 | (14) |
|
|
||||||
| UC HII | ||||||
|
|
||||||
| G5.89–0.39b | 18:00:30.5 | −24:04:01 | + 9.0 | 1.28 | 105.1 | (15, 16) |
| I19035-VLA1b | 19:06:01.5 | +06:46:35 | + 32.4 | 2.2 | 103.9 | (11) |
| 19410+2336a | 19:43:11.4 | +23:44:06 | + 22.4 | 2.1 | 104.0 | (17) |
| ON1a | 20:10:09.1 | +31:31:36 | + 12.0 | 2.5 | 104.3 | (18, 19) |
| I22134-VLA1a | 22:15:09.2 | +58:49:08 | −18.3 | 2.6 | 104.1 | (11) |
| 23033+5951a | 23:05:24.6 | +60:08:09 | −53.0 | 3.5 | 104.0 | (17) |
| NGC 7538-IRS9a | 23:14:01.8 | +61:27:20 | −57.0 | 2.8 | 104.6 | (8) |
Notes. Column 4 shows the velocity at which we centred the spectra, corresponding to the systemic velocity. Columns 5 and 6 give the source distance and bolometric luminosity (respectively) of the associated star forming region. This latter is a very rough first approximation of the core luminosity because it is based on infrared measurements having poor angular resolution. We adopt as source names those used in the reference papers listed in Col. 7.
Luminosity of the core and not of the whole associated star-forming region (Rathborne et al. 2010).
References.
Palau et al. (2010);
Busquet et al. (2011);
Beuther et al. (2007b);
Butler & Tan (2009);
Palau et al. (2007);
Busquet et al. (2010);
Busquet (2010);
Sánchez-Monge et al. (2008);
Beuther et al. (2004);
Schnee & Carpenter (2009);
Sánchez-Monge (2011);
Ando et al. (2011);
Fontani et al. (2004a);
Fontani et al. (2004b);
Hunter et al. (2008);
Motogi et al. (2011);
Beuther et al. (2002);
Su et al. (2009);
Nagayama et al. (2011);
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