Table 6
Properties of the detected methanol line sources.
| ID | GLOSTAR name | SIMBAD or Common name | Possible | 1.2 mm | 6-GHz | VLSR (a) | VLSR |
|---|---|---|---|---|---|---|---|
| nature | core(b) | continuum | (km s−1) | Ref. | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| 1 | G76.0932+0.1580 | J202323.73+373535.16(c) | pre-UC HII | – | – | 0.7 | 1 |
| 2 | G76.8437+0.1233 | J202543.79+381112.98(c) | pre-UC HII | – | – | –4.4 | 1 |
| 3 | G78.8870+0.7087 | AFGL2591 | UC HII region | S26 | yes | –5.7 | 2 |
| 4 | G78.9690+0.5410 | IRAS 20286+3959 | pre-UC HII | – | – | 7.0 | 3 |
| 5 | G78.9884+0.2211 | J203147.25+395900.33(c) | pre-UC HII | – | – | –62.8 | 4 |
| 6 | G79.7358+0.9904 | IRAS 20290+4052 | pre-UC HII | – | – | –1.4 | 5 |
| 7 | G80.8617+0.3834 | DR20, IRAS 20352+4124 | UC or HC HII region | N14 | yes | –1.5 | 6 |
| 8(d) | G81.6790+0.5378 | DR21 | UC HII region | N46 | yes | –3.0 | 7 |
| 9 | G81.7219+0.5711 | DR21(OH) | UC HII region | N44 | yes | –2.6 | 3 |
| 10 | G81.7444+0.5910 | W75S-FIR1, DR21 B | UC or HC HII region | N43 | yes | –3.1 | 7 |
| 11 | G81.7523+0.5908 | W75S-FIR2, DR21 A | High-luminosity IR protostellar core | N51 | – | –3.3 | 7 |
| 12 | G81.7655+0.5972 | CygX-N53 | Massive IR-quiet protostellar core | N53 | – | –4.4 | 8 |
| 13 | G81.8713+0.7807 | W75N(B) | UC HII region | N30 | yes | 12.0 | 9 |
| 14 | G82.3079+0.7296 | J204016.75+425629.49(c) | pre-UC HII | – | – | 11.4 | 1 |
Notes. (a) Systemic LSR velocity of moleculargas. (b)From Motte et al. (2007). (c)From Kryukova et al. (2014). (d)Seen in absorption. References. 1. Schneider et al. (2006); 2. van der Tak et al. (1999); 3. Keown et al. (2019); 4. Yamagishi et al. (2018); 5. Bronfman et al. (1996); 6. Pipenbrink & Wendker (1988); 7. This work; 8. Duarte-Cabral et al. (2014); 9. Gottschalk et al. (2012).
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