Table 1
Sources with detections of at least one of the COMs studied in this work (MF, DE, F, and EC), sorted by evolutionary stage.
| Source | α(J2000) | δ(J2000) | d | L | M | References |
|---|---|---|---|---|---|---|
| (h : m : s) | (°: ′ : ′′) | (kpc) | (L⊙) | (M⊙) | ||
| HMSC | ||||||
| 05358-mm3 | 05: 39: 12.5 | +35 : 45 : 55 | 1.8 | 103.8 | 101.9 | (1, 6, 31, 32, 33, 34, 35, 36) |
| HMPO | ||||||
| AFGL5142-MM | 05: 30 : 48.0 | +33 : 47 : 54 | 1.8 | 103.6 | 101.8 | (1, 6, 31, 32, 33, 34, 35, 36) |
| 18182-1433M1 | 18 : 21 : 09.2 | −14 : 31 : 49 | 4.5 | 104.0 | 102.5 | (2, 3, 4, 34) |
| 18517+0437 | 18 : 54 : 14.2 | +04 : 41 : 41 | 2.9 | 104.1 | 102.1 | (1, 6, 30, 31, 32, 33, 34, 35, 36) |
| I20293-MM1 | 20 : 31 : 12.8 | +40 : 03 : 23 | 2.0 | 103.6 | 101.6 | (1, 6, 30, 31, 32, 33, 35) |
| I23385 | 23 : 40 : 54.5 | +61 : 10 : 28 | 4.9 | 104.2 | 102.1 | (1, 6, 30, 31, 32, 33, 35) |
| INT | ||||||
| 18089-1732 | 18 : 11 : 51.4 | −17 : 31 : 28 | 3.6 | 104.5 | 102.4 | (1, 6, 9, 30, 31, 32, 33, 34, 35, 36) |
| G24.78+0.08 | 18 : 36 : 12.6 | −07 : 12 : 11 | 7.7 | 105.3 | 103.5 | (2, 10, 11, 34) |
| G31.41+0.31 | 18 : 47 : 34.2 | −01 : 12 : 45 | 3.8 | 104.6 | 102.9 | (2, 7, 8, 29, 34, 38) |
| 20126+4104M1 | 20 : 14 : 25.9 | +41 : 13 : 34 | 1.7 | 104.0 | 102.9 | (2, 12, 13, 29, 34, 37, 39) |
| G75-core | 20 : 21 : 44.0 | +37 : 26 : 38 | 3.8 | 104.8 | 102.1 | (1, 2, 5, 6, 30, 31, 32, 33, 34, 35, 36) |
| UCHII | ||||||
| W3(OH) | 02 : 27 : 04.7 | +61 : 52 : 25 | 2.0 | 105.0 | 101.5 | (16, 20, 21, 22, 34) |
| G5.89-0.39 | 18 : 00 : 30.5 | −24 : 04 : 01 | 1.3 | 105.1 | 102.3 | (1, 6, 29, 30, 31, 32, 33, 34, 35, 36) |
| G10.47+0.03 | 18 : 08 : 38.0 | −19 : 51 : 50 | 5.8 | 106.1 | 103.2 | (17, 18, 19, 29, 34) |
| G14.33-0.65 | 18 : 18 : 54.8 | −16 : 47 : 53 | 2.6 | 104.3 | 102.5 | (2, 23, 24, 34) |
| G29.96-0.02 | 18 : 46 : 03.0 | −02 : 39 : 22 | 8.9 | 105.8 | 103.9 | (10, 15, 16, 29, 34) |
| G35.20-0.74 | 18 : 58 : 13.0 | +01 : 40 : 36 | 2.2 | 104.5 | 102.2 | (2, 25, 26, 27, 28, 34) |
| W51 | 19 : 23 : 43.9 | +14 : 30 : 32 | 5.4 | 106.7 | 102.8 | (7, 14, 34) |
| 19410+2336 | 19 : 43 : 11.4 | +23 : 44 : 06 | 2.1 | 104.0 | 102.1 | (1, 2, 6, 30, 31, 32, 33, 34, 35, 36) |
| ON1 | 20 : 10 : 09.1 | +31 : 31 : 36 | 2.5 | 104.3 | 102.5 | (1, 2, 6, 30, 31, 32, 33, 34, 35, 36) |
Notes. Distances from the Sun and bolometric luminosities are taken from literature (see references), while masses have been derived from the molecular hydrogen column densities of the sources from the literature (see Table 4 and Sect. 6.3 for details).
References. (1) Fontani et al. (2011); (2) Colzi et al. (2018b); (3) Rosero et al. (2016); (4) Beuther et al. (2006); (5) Murphy et al. (2010); (6) Fontani et al. (2015a); (7) Rivilla et al. (2017a); (8) De Buizer (2003); (9) Lackington (2011); (10) Cesaroni et al. (2017); (11) Beltrán et al. (2007); (12) Beltrán & de Wit (2016); (13) Cesaroni et al. (1999); (14) Etoka et al. (2012); (15) Kirk et al. (2010); (16) Hoare et al. (2007); (17) Pascucci et al. (2004); (18) López-Sepulcre et al. (2009); (19)Hatchell et al. (2000); (20)Fish & Sjouwerman (2007); (21)Mueller et al. (2002); (22)Wyrowski et al. (1997); (23)Liu et al. (2010); (24)Walsh et al. (1997); (25)Caratti o Garatti et al. (2015); (26)Zhang et al. (2014); (27)Sánchez-Monge et al. (2013); (28)De Buizer (2006); (29)Fontani et al. (2007); (30)Fontani et al. (2014); (31)Fontani et al. (2015b); (32)Fontani et al. (2016); (33)Fontani et al. (2018); (34)Fontani et al. (2019); (35)Colzi et al. (2018a); (36)Mininni et al. (2018); (37)Cesaroni et al. (1997); (38)Immer et al. (2019); (39)Fontani et al. (2006).
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