Table 4.
Extended H II regions in the λ6 cm survey.
| No. | G-NAME | GLong6 cm | GLat6 cm | Apparent θmaj | Apparent θmin | S6 cm | GLongwise | GLatwise | Diameter | D | Ref. | Notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (°) | (°) | (′) | (′) | (Jy) | (°) | (°) | (′) | (kpc) | ||||
| 1 | G11.7−1.7 | 11.69 | −1.74 | 19.8 | 15.7 | 5.084 | 11.662 | −1.692 | 30.2 | 1.6 ± 0.2 | rus03 | SH 2-37, P150 |
| 2 | G13.8−0.8 | 13.80 | −0.81 | 18.0 | 11.5 | 12.183 | 13.776 | −0.795 | 18.1 | RCW 156, P176 | ||
| 3 | G15.1+3.3 | 15.11 | 3.35 | 22.0 | 20.3 | 7.743 | 15.128 | 3.310 | 37.8 | 2.8 ± 0.6 | rus03 | SH 2-46, P202 |
| 4 | G16.9−1.1 | 16.87 | −1.05 | 21.8 | 13.9 | 7.447 | 16.857 | −1.155 | 23.9 | SH 2-50, including P216, see Sun et al. (2011b) | ||
| 5 | G16.9+0.8 | 16.94 | 0.77 | 60 | 55 | 162.677 | 16.993 | 0.874 | 37.5 | 2.0 ± 0.25 | rus03 | SH 2-49, RCW 165, P218,P219,P220,P224 |
| ⋯ | ||||||||||||
| 75 | G17.0+1.7 | 17.02 | 1.72 | 27.8 | 15.7 | 6.353 | P221/P222, flat radio spectrum | |||||
| 76 | G20.3−0.9 | 20.27 | −0.89 | 18.5 | 13.0 | 3.560 | P266/P267/P268, flat radio spectrum | |||||
| 77 | G63.7−0.7 | 63.65 | −0.72 | 17.0 | 13.6 | 0.858 | P622, flat radio spectrum | |||||
| 78 | G66.4−1.2 | 66.41 | −1.17 | 100 | 96 | 7.874 | 66.660 | −1.167 | 62.5 | DU 34, including P631, Q-type WISE H II region? | ||
| 79 | G68.4+0.2 | 68.39 | 0.19 | 23.6 | 17.3 | 1.404 | flat radio spectrum, possible infrared emission associated | |||||
| ⋯ |
Notes. Columns 1 and 2: sequential number and G-name; Cols. 3 and 4: Galactic longitude and latitude of the λ6 cm source; Cols. 5 and 6: apparent size θmaj and θmin of the λ6 cm source measured in Galactic longitude and latitude directions; Col. 7: integrated flux density at λ6 cm; Cols. 8 and 9: Galactic longitude and latitude of the matched WISE H II region; Col. 10: diameter of the matching WISE H II region; Cols. 11 and 12: distance information and their references; Col. 13: remarks for the source. Some other references in the 13th column: e.g. Sieber & Seiradakis (1984), Suad et al. (2012), Gao et al. (2011), Gao & Han (2013) and Graham et al. (1982). Full table is accessible from the CDS.
References. abb+14: Anderson et al. (2014); aaj+15: Anderson et al. (2015); aal+18: Anderson et al. (2018); rmb+09: Reid et al. (2009); chr+14: Choi et al. (2014); fb84: Fich & Blitz (1984); fb15: Foster & Brunt (2015); hh14: Hou & Han (2014); rus03: Russeil (2003); rag07: Russeil et al. (2007).
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