Table 3
Bolometric, H2O maser, and radio luminosites of prototypical jets associated with H2O maser sites (Fig. 5; cyan circles).
| Source | D | Lbol |  |
L8 GHz | References |
|---|---|---|---|---|---|
| (kpc) | (104 L⊙) | (10−5 L⊙) | (mJy kpc2) | ||
| Cepheus A HW2 | 0.7 | 2.4 | 4.50 | 3.24 | 1,2,3,4,5 |
| HH 80-81 | 1.7 | 1.7 | 1.41 | 8.47 | 6,3,7,8,9 |
| IRAS 20126 | 1.6 | 1.3 | 0.39 | 0.38 | 10,2,11,12 |
| S255 NIRS3 | 1.8 | 2.9 | 0.42 | 3.28 | 13,14,15,16 |
| AFGL 5142 MM1 | 2.1 | ... | 0.86 | 3.33 | 17,15,18,19 |
| AFGL 2591 VLA–3 | 3.3 | 23 | 1.20 | 16.15 | 20,21,22 |
| G023.01−0.41 | 4.6 | 4.0 | 6.46 | 8.97 | 23,24,25,26,27 |
Notes. Sources are listed by increasing heliocentric distance. Column 2: distances to the Sun. Column 3: bolometric luminosities associated with (and dominated by) individual young stars. For region AFGL 5142, a reliable estimate of the bolometric luminosity for source MM1 is not available, and this source has not been plotted in Fig. 5 b. Column 4: H2O maser luminosities for Cepheus A HW2 and HH 80-81 are from Furuya et al. (2003); all other values were obtained from accurate VLBA measurements that our group conducted in recent years. Column 5: radio continuum luminosities at 8 GHz. Column 6: references to the papers used for estimating values in Cols. 2–5.
References. (1) Moscadelli et al. (2009); (2) De Buizer et al. (2017); (3) Furuya et al. (2003); (4) Rodriguez et al. (1994); (5) Curiel et al. (2006); (6) Rodriguez et al. (1980); (7) Marti et al. (1993); (8) Carrasco-González et al. (2010); (9) Rodríguez-Kamenetzky et al. (2017); (10) Moscadelli et al. (2011); (11) Chen et al. (2016); (12) Hofner et al. (2007); (13) Burns et al. (2016); (14) Caratti o Garatti et al. (2017); (15) Goddi et al. (2007); (16) Cesaroni et al. (2018); (17) Burns et al. (2017); (18) Goddi & Moscadelli (2006); (19) Goddi et al. (2011); (20) Rygl et al. (2012); (21) Sanna et al. (2012); (22) Johnston et al. (2013); (23) Brunthaler et al. (2009); (24) Sanna et al. (2014); (25) Sanna et al. (2010b); (26) Sanna et al. (2016); (27) Rosero et al. (2016).
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