Table 1.
Source parameters from the CORE sample (as listed in Beuther et al. 2018).
| Source | RA (J2000) (h:min:s) | Dec (deg:′:″) | D (kpc) | Ma (M⊙) | vlsr (km s−1) | L (104 L⊙) |
|---|---|---|---|---|---|---|
| G75.78+0.34 | 20:21:44.03 | +37:26:37.70 | 3.8d | 13 490 | −0.5d | 7.0f |
| IRAS21078+5211 | 21:09:21.64 | +52:22:37.50 | 1.5b | 410 | −6.1b | 1.3b |
| NGC7538 IRS1 | 23:13:45.36 | +61:28:10.55 | 2.7c | 12 000 | −57.3c, e | 8.0f |
Notes. aThe masses are estimated for the entire regions covered by the 1.2 mm dust continuum maps assuming optically thin dust emission at a temperature of 20 K (see also Section 3.1). b: Molinari et al. 1996, c: Reid et al. 2009, d: Ando et al. 2011, e: Moscadelli et al. 2009, f: RMS survey database (http://rms.leeds.ac.uk/cgi-bin/public/RMS_DATABASE.cgi).
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