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Table 2

Candidate HC H II regions.

S.No. GLOSTAR name CORNISH name Separation(*) ΔV α(**) deff (***)
(″) (km s−1) (pc)
1 G010.624−0.384 G010.6234−00.3837 2.43 38.69 ± 1.6 0.97 1.24
2 G010.302−0.147 G010.3009−00.1477 4.75 38.36 ± 1.79 0.31 0.78
3 G011.937−0.615 G011.9368−00.6158 2.89 40.52 ± 1.89 0.36 0.71
4 G012.805−0.200 G012.8050−00.2007 2.41 37.63 ± 0.5 0.84 0.88
5 G013.210−0.144 G013.2099−00.1428 4.3 36.39 ± 1.72 0.61 1.15
6 G016.944−0.074 G016.9445−00.0738 1.92 43.81 ± 4.64 0.55 3.65
7 G026.544+0.415 G026.5444+00.4169 6.96 36.92 ± 2.5 0.25 3.74
8 G028.287−0.364 G028.2879−00.3641 3.22 39.27 ± 5.38 0.23 0.7
9 G029.957−0.017 G029.9559−00.0168 4.22 39.92 ± 1.33 0.52 1.31
10 G030.535+0.021 G030.5353+00.0204 2.42 36.77 ± 1.76 0.2 3.05
11 G034.257+0.153 G034.2572+00.1535 2.06 59.79 ± 2.6 1.22 0.77
12 G037.874−0.399 G037.8731−00.3996 3.97 43.73 ± 1.59 0.55 2.59
13 G043.165−0.029 G043.1651−00.0283 2.62 40.06 ± 1.16 1.23 1.93
14 G045.122+0.131 G045.1223+00.1321 4.0 57.83 ± 1.64 0.63 1.47
15 G049.490−0.369 G049.4905−00.3688 2.03 38.4 ± 0.83 0.93 0.61

Notes. (*)Angular separation between GLOSTAR and CORNISH peak emission. (**)Spectral index between 1.4–5 GHz as reported by Yang et al. (2019). (***) deff represents the effective diameter of the source (refer to Sect. 4.3.2), and these values might exceed the true size of the sources.

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