Table C.1
GLOSTAR H II region catalog with continuum and stacked ⟨Hnα⟩ hydrogen RRL parameters.
| Name(a) | GLOSTAR Name(b) | ℓpeak [°] | bpeak [°] | Speak [Jy Beam−1] | Sc [mJy] | σSc [mJy] | SL [mJy] | σSL [mJy] | ΔV [km s−1] | σΔV [km s−1] | VLSR [km s−1] | σVLSR [km s−1] | Dsun (c) [kpc] | σ Dsun [kpc] | RGal [kpc] | Morphology(d) | ATLASGAL Clump(e) | CH3OH(f) |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | |
| · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | |
| · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | |
| · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | |
| G031.474-0.344 | G031.476-00.344 | 31.474 | −0.344 | 0.07 | 261.75 | 14.24 | 26.27 | 3.94 | 28.84 | 5.0 | 89.62 | 2.12 | 9.0 | 0.7 | 4.72 | IB | ... | ... |
| G032.059+0.080 | G032.063+00.078 | 32.059 | 0.08 | 0.03 | 157.28 | 11.34 | 21.23 | 3.23 | 23.9 | 4.19 | 98.86 | 1.78 | 7.2 | 0.0 | 4.34 | B | ... | ... |
| G032.150+0.133 | G032.151+00.133 | 32.15 | 0.133 | 0.51 | 681.96 | 34.22 | 46.24 | 1.99 | 26.49 | 1.32 | 97.46 | 0.56 | 6.2 | 0.62 | 4.39 | IB | AGAL032.149+00.134 | ... |
| G032.272-0.225 | G032.272-00.226 | 32.272 | −0.225 | 0.29 | 320.89 | 16.15 | 12.57 | 1.31 | 23.59 | 2.85 | 21.34 | 1.21 | 12.8 | 0.5 | 7.34 | C | AGAL032.272-00.226 | ... |
| G032.589+0.008 | G032.590+00.010 | 32.589 | 0.008 | 0.02 | 173.41 | 9.78 | 20.59 | 3.87 | 15.95 | 3.46 | 80.37 | 1.47 | 9.4 | 0.6 | 5.07 | PB | ... | ... |
| G032.797+0.191 | G032.798+00.191 | 32.797 | 0.191 | 2.71 | 3129.42 | 156.55 | 121.92 | 2.15 | 33.04 | 0.67 | 16.18 | 0.29 | 9.71 | 2.92 | 5.26 | C | AGAL032.797+00.191 | G032.8027+0.1926 |
| G032.927+0.606 | G032.928+00.606 | 32.927 | 0.606 | 0.29 | 328.51 | 16.51 | 12.7 | 2.24 | 27.42 | 5.58 | −34.95 | 2.37 | 19.2 | 1.5 | 13.13 | C | AGAL032.926+00.606 | |
| G032.990+0.040 | G032.991+00.039 | 32.99 | 0.04 | 0.14 | 188.07 | 10.79 | 17.69 | 2.05 | 22.82 | 3.06 | 91.56 | 1.3 | 8.6 | 0.86 | 4.78 | B | ... | G032.9918+0.0343 |
| G033.204-0.009 | IRAS 18494+0010 | 33.204 | −0.009 | 0.09 | 374.08 | 21.28 | 31.7 | 3.51 | 22.51 | 2.87 | 107.49 | 1.22 | 7.1 | 0.71 | 4.47 | IB | AGAL033.206-00.009 | G033.2037-0.0101 |
| G033.419-0.004 | G033.418-00.004 | 33.419 | −0.004 | 0.13 | 196.04 | 10.33 | 10.93 | 1.4 | 34.3 | 5.07 | 63.49 | 2.15 | 9.4 | 0.94 | 5.19 | C | ... | ... |
| G033.810-0.189 | G033.810-00.188 | 33.81 | −0.189 | 0.22 | 309.83 | 15.68 | 18.57 | 2.59 | 21.13 | 3.4 | 39.6 | 1.45 | 11.7 | 1.17 | 6.7 | PB | AGAL033.811-00.187 | ... |
| G033.915+0.110 | G033.914+00.110 | 33.915 | 0.11 | 0.82 | 991.23 | 49.67 | 52.58 | 1.86 | 34.62 | 1.42 | 100.02 | 0.6 | 7.1 | 0.71 | 4.56 | IB | AGAL033.914+00.109 | ... |
| G034.089+0.436 | GO34.089+00.436 | 34.089 | 0.436 | 0.11 | 241.65 | 12.99 | 19.24 | 3.04 | 16.95 | 3.09 | 34.26 | 1.31 | 12.2 | 1.22 | 7.11 | IB | AGAL034.089+00.436 | ... |
| GO34.132+0.471 | G034.133+00.471 | 34.132 | 0.471 | 0.41 | 518.68 | 26.22 | 30.94 | 3.03 | 21.16 | 2.39 | 34.4 | 1.02 | 11.7 | 0.5 | 6.74 | B | AGAL034.133+00.471 | ... |
| GO34.255+0.146 | CORNISH G034.2544+00.1460 | 34.255 | 0.146 | 2.25 | 8087.97 | 405.24 | 532.43 | 6.7 | 25.25 | 0.37 | 54.04 | 0.16 | 3.4 | 0.34 | 5.67 | IB | ... | ... |
| GO34.257+0.153(*) | CORNISH G034.2573+00.1523 | 34.257 | 0.153 | 2.29 | 2440.25 | 122.65 | 39.35 | 1.48 | 59.79 | 2.6 | 44.09 | 1.1 | 3.4 | 0.34 | 5.67 | C | AGAL034.258+00.154 | G34.2582+0.1534 |
| GO34.322+0.160 | ... | 34.322 | 0.16 | 0.03 | 102.1 | 17.61 | 13.67 | 1.22 | 31.49 | 3.23 | 53.8 | 1.37 | 10.4 | 0.35 | 5.88 | ND | ... | ... |
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Notes. The entire table is accessible in a machine-readable format at the CDS. A section of the table is provided here as a reference for its format and content. (a)Glll.lll+b.bbb where 1 and b is the position of peak pixel. (b)Name of the corresponding GLOSTAR continuum source located within angular separations of 36″ in the GLOSTAR VLA D-conflguration continuum source catalog (Medina et al. 2019, 2024). For sources where no crossmatch was found due to contamination from extended large-scale structures, we provided the name of the nearest H II region in the SIMBAD database. (c)References for distances: (1) Reid et al. (2019); (2) Anderson et al. (2012); (3) Anderson & Bania (2009); (4) Urquhart et al. (2018). (d)Classification of source based on Spitzer GLIMPSE 8 μm emissions, as is explained in Section. 5.1. (e)Name of the associated ATLASGAL dust clump (Urquhart et al. 2014) (see Section. 5.2). (f)Name of the associated 6.7 GHz methanol (CH3OH) maser (Nguyen et al. 2022) (see Section. 5.3). (*)Candidate HC H II regions (see Section. 4.3.2).
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