Table 1
Hii regions from the WISE and Sharpless catalogs.
| WISE | Sh2-no. | GLON | GLAT | Radius (arcsec) | MWSC | Vlsr (km s−1) | Vmlsr (km s−1) | Mol | Dist. (kpc) | Dist. (OA) (kpc) | Notes |
|---|---|---|---|---|---|---|---|---|---|---|---|
| G118.621−01.329 | 172 | 118.621 | −1.329 | 235 | BDSB 48 | −42.6 | −39.2 | NH3 | 4.3 | 3.12 ± 0.34(a) | G |
| G118.629−00.406 | − | 118.629 | −0.406 | 136 | − | − | − | − | − | F | |
| G118.928−03.337 | − | 118.928 | −3.336 | 126 | FSR 0486 | − | − | − | − | I | |
| G118.959−03.321 | − | 118.959 | −3.32 | 82 | FSR 0486 | − | − | − | − | I | |
| G118.977−03.345 | − | 118.977 | −3.345 | 104 | FSR 0486 | − | − | − | − | I | |
| G119.220−02.463 | − | 119.220 | −2.462 | 85 | − | − | − | − | − | H | |
| G119.437−00.916 | 173 | 119.437 | −0.916 | 1068 | Mayer 1 | −34.3 | − | − | 3.4 | 3.12 ± 0.34(a) 2.96 ± 0.31(b) | E |
| G119.558+00.645 | − | 119.558 | 0.646 | 83 | − | − | −51.9 | 12CO | − | D | |
| G119.800−06.007 | − | 119.800 | −6.007 | 329 | − | − | − | − | − | K | |
| G120.495+00.077 | − | 120.495 | 0.077 | 298 | − | − | − | − | − | C | |
| G121.276−01.036 | − | 121.276 | −1.035 | 287 | − | − | − | − | − | A | |
| G121.297+00.658 | − | 121.298 | 0.659 | 141 | − | − | −17.7 | CS | 0.9 | Y | |
| G122.002−07.084 | 122.002 | −7.083 | 235 | − | − | − | − | 2.1 |  (c) |
L | |
| G122.459−00.781 | − | 122.459 | −0.78 | 188 | − | − | −42.8 | NH3 | 4.2 | ||
| X | |||||||||||
| G123.155−06.306 | 184 | 123.155 | −6.306 | 1093 | IC 1590 | −29.7 | − | − | 2.8 |  (c) 3.1 ± 0.13(b) |
M |
| G123.809−01.781 | 185 | 123.809 | −1.781 | 73 | − | − | −31.9 | 13CO | 3.1 | 3.23 ± 0.65(b) | S |
| G123.836−01.762 | 185 | 123.836 | −1.761 | 1250 | − | − | − | − | 3.23 ± 0.65(b) | S | |
| G123.936−06.472 | − | 123.936 | −6.472 | 826 | − | − | − | − | − | N | |
| G124.037+00.051 | − | 124.037 | 0.051 | 171 | − | − | − | − | − | 1.9 ± 0.6(d) | V |
| G124.859+00.323 | − | 124.859 | 0.324 | 95 | BDSB 51 | − | − | − | − | U | |
| G124.860−05.705 | − | 124.860 | −5.704 | 1183 | − | − | − | − | − | O | |
| G124.870−03.135 | − | 124.870 | −3.134 | 371 | − | − | − | − | − | R | |
| G124.894+00.323 | 186 | 124.894 | 0.323 | 226 | BDSB 51 | −41.2(e) | − | − | 4.0(e) | 2.76 ± 0.2(b) 4.1 ± 0.8(f) | U |
| G124.937+00.077 | − | 124.937 | 0.078 | 1413 | − | − | − | − | − | U | |
| G124.937−00.248 | − | 124.937 | −0.247 | 118 | − | − | −43.3 | 12CO | − | T | |
| G124.977−04.062 | − | 124.978 | −4.061 | 118 | − | − | − | − | − | Q | |
| G125.137−04.067 | − | 125.137 | −4.067 | 197 | − | − | − | − | − | Q | |
| G125.602−05.207 | − | 125.602 | −5.207 | 421 | − | − | − | − | − | M | |
| Sharpless | Diam (arcmin) | − | − | − | − | − | |||||
| Sh2−172 | − | 118.6 | −1.3 | 1 | − | − | − | − | − | G | |
| Sh2−173 | − | 119.5 | −0.9 | 30 | − | − | − | − | − | 2.96 ± 0.31(b) | E |
| Sh2−176 | − | 120.3 | −5.5 | 10 | − | − | − | − | − | 0.10 ± 0.03(g) | J |
| Sh2−177 | − | 120.7 | −0.3 | 40 | − | − | − | − | − | 3.12 ± 0.34(a) 2.37 ± 0.22(b) | B |
| Sh2−179 | − | 121.7 | 0.0 | 1 | − | − | − | − | − | Z | |
| Sh2−180 | − | 122.6 | 0.1 | 15 | − | − | − | − | − | 5.41 ± 1.08(b) | W |
| Sh2−184 | − | 123.1 | −6.3 | 40 | − | − | − | − | − | 3.10 ± 0.13(b) | M |
| Sh2−185 | − | 124.0 | −1.9 | 120 | − | − | − | − | − | 3.23 ± 0.65(b) | S |
| Sh2−186 | − | 124.9 | 0.3 | 1 | − | − | − | − | 2.76 ± 0.2(b) 4.1 ± 0.8(f) | U |
References. (a) Russeil et al. (2007). (b) Foster & Brunt (2015). (c) For the region, G122.002−07.084 Wenger et al. (2018) derived the kinematic distance using three different methods: the traditional method using the Brand & Blitz (1993) rotation curve and the IAU-defined solar motion parameters (Method A, dA = 5.00 ± 1.18), the traditional method using the Reid et al. (2014) rotation curve and their revised solar motion parameters (Method B, dB = 4.10 ± 0.92), and a new Monte Carlo method using the Reid et al. (2014) rotation curve and their revised solar motion parameters (Method C, 
). For the region G123.155−06.30, Wenger et al. (2018) derived dA = 2.91 ± 1.19, dB = 2.37 ± 0.95, and 
. (d) Kerton (2002).(e) Anderson et al. (2015). (f) Balser et al. (2011). (g) Sabbadin et al. (1977).
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