Table 1
Source sample.
| Source | RA (J2000.0) | Dec | V LSR | L bol | d | Ref. |
| h m s | ° ′ ′′ | km s-1 | L ⊙ | kpc | ||
|
|
||||||
| Mid-IR-quiet HMPOs | ||||||
| IRAS 05358+3543 | 05 39 13.1 | +35 45 50 | −17.6 | 6.3 × 103 | 1.8 | 1, 1 |
| IRAS 16272–4837 | 16 30 58.7 | −48 43 55 | −46.2 | 2.4 × 104 | 3.4 | 2, 2 |
| NGC 6334I(N) | 17 20 55.2 | −35 45 04 | −4.5 | 1.9 × 103 | 1.7 | 3, 4 |
| W43 MM1 | 18 47 47.0 | −01 54 28 | +98.8 | 2.3 × 104 | 5.5 | 5, 6 |
| DR21(OH) | 20 39 00.8 | +42 22 48 | −4.5 | 1.3 × 104 | 1.5 | 7, 8 |
| Mid-IR-bright HMPOs | ||||||
| W3 IRS5 | 02 25 40.6 | +62 05 51 | −38.4 | 1.7 × 105 | 2.0 | 9, 10 |
| IRAS 18089–1732 | 18 11 51.5 | −17 31 29 | +33.8 | 1.3 × 104 | 2.3 | 11, 12 |
| W33A | 18 14 39.1 | −17 52 07 | +37.5 | 4.4 × 104 | 2.4 | 11, 30 |
| IRAS 18151–1208 | 18 17 58.0 | −12 07 27 | +32.0 | 2.0 × 104 | 2.9 | 13, 13 |
| AFGL 2591 | 20 29 24.7 | +40 11 19 | −5.5 | 2.2 × 105 | 3.3 | 14, 8 |
| Hot molecular cores | ||||||
| G327−0.6 | 15 53 08.8 | −54 37 01 | −45.0 | 5.0 × 104 | 3.3 | 15, 16 |
| NGC 6334I | 17 20 53.3 | −35 47 00 | −7.7 | 2.6 × 105 | 1.7 | 3, 4 |
| G29.96−0.02 | 18 46 03.8 | −02 39 22 | +98.7 | 3.5 × 105 | 6.0 | 17, 18 |
| G31.41+0.31 | 18 47 34.3 | −01 12 46 | +98.8 | 2.3 × 105 | 7.9 | 19, 20 |
| Ultracompact Hii regions | ||||||
| G5.89−0.39 (W28A) | 18 00 30.4 | −24 04 02 | +10.0 | 5.1 × 104 | 1.3 | 21, 22 |
| G10.47+0.03 | 18 08 38.2 | −19 51 50 | +67.0 | 3.7 × 105 | 5.8 | 23, 20 |
| G34.26+0.15 | 18 53 18.6 | +01 14 58 | +57.2 | 3.2 × 105 | 3.3 | 24, 25 |
| W51N-e1 | 19 23 43.8 | +14 30 26 | +59.5 | 1.0 × 105 | 5.1 | 26, 27 |
| NGC 7538-IRS1 | 23 13 45.3 | +61 28 10 | −57.4 | 1.3 × 105 | 2.7 | 28, 29 |
Notes.The first reference is for the luminosity, the second for the distance. If the distance measurement is more recent than the luminosity estimate, the luminosity has been scaled to the new distance. The text uses “short” source names, which is the part preceding the + or − sign.
Reference. (1) Beuther et al. (2002); (2) Garay et al. (2002); (3) Sandell (2000); (4) Neckel (1978); (5) Nguyen Luong et al. (2011); (6) Lester et al. (1985); (7) Jakob et al. (2007); (8) Rygl et al. (2012); (9) Ladd et al. (1993); (10) Hachisuka et al. (2006); (11) Faúndez et al. (2004); (12) Xu et al. (2011); (13) Sridharan et al. (2002); (14) Van der Tak et al. (1999); (15) Urquhart et al. (2012); (16) Minier et al. (2009); (17) Cesaroni et al. (1998); (18) Pratap et al. (1999); (19) Mueller et al. (2002); (20) Churchwell et al. (1990); (21) Van der Tak et al. (2000) (22) Motogi et al. (2011); (23) Hunter et al. (2000); (24) Hatchell & van der Tak (2003) (25) Kuchar & Bania (1994); (26) Van Dishoeck et al. (2011); (27) Xu et al. (2009); (28) Sandell & Sievers (2004); (29) Moscadelli et al. (2009); (30) Immer et al. (2013).
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