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Table 2.

Small-diameter H II regions identified in the Urumqi λ6 cm survey by comparison with the Paladini H II region catalogue.

P number G-NAME GLong GLat Ref. D Ref. EB S21cm EB S11cm Urumqi S6cm SRef Freq Ref. Notes
(°) (°) (kpc) (Jy) (Jy) (Jy) (Jy) (GHz)
129 G10.1−0.4 10.073 −0.412 A78 4.95 ± 0.51 srm+14 47.01 54.819 63.835 3.00 4.9 A78 Included in the λ6 cm source G10.16−0.35
3.0 4.9 D80
131 G10.2−0.4 10.190 −0.426 D80 4.95 ± 0.51 srm+14 47.01 54.819 63.835 5.1 4.9 D80 Included in the λ6 cm source G10.16−0.35
132 G10.2−0.3 10.159 −0.349 K97 4.95 ± 0.51 srm+14 47.01 54.819 63.835 55 2.7 A70 Included in the λ6 cm source G10.16−0.35
65 2.7 G70 New 14.7 GHz flux density
66.353 4.9 K97
47 5.0 A70
47.48 4.9 A78
47.5 4.9 D80
63.2 5.0 M67
51.8 5.0 R70
48.4 5.0 Wil70
31.67 10.0 H87
<36.6 14.7 W83
134 G10.3−0.2 10.315 −0.150 K97 4.95 ± 0.51 srm+14 14.61 13.77 15.923 22 2.7 G70 Same as P135
20.472 4.9 K97
12.48 4.9 A78
12.5 4.9 D80
20.2 5.0 M67
<9.2 14.7 W83
135 G10.3−0.1 10.307 −0.145 R70 14.61 13.77 15.923 20 2.7 A70 Same as P134
20 5.0 A70
13.6 5.0 R70
10.81 10.0 H87

Notes. Column 1: sequential number in Paladini et al. (2003); Col. 2: G-name of the H II region; Cols. 3, 4 and 5: Galactic longitude, latitude and their reference; Cols. 6 and 7: distance for the H II region and reference; Cols. 8, 9 and 10: integrated flux densities based on the Effelsberg λ21 cm, λ11 cm and the Urumqi λ6 cm data. Some of the λ11 cm results (with 2 digits) are from the data at original resolution and some (with 3 digits) are from the data which were convolved to an angular resolution of ; Cols. 11, 12 and 13: integrated flux densities, the corresponding frequencies and their references. Most of these are based on Paladini et al. (2003), except those of Handa et al. (1987). The flux densities from Paladini et al. (2003) were all examined by comparing the results to the original references. Corrections were made if improper values were found; Col. 14: remarks for the source. Full table is accessible from the CDS.

References. brm+09: Brunthaler et al. (2009); chr+14: Choi et al. (2014); fb84: Fich & Blitz (1984); fb15: Foster & Brunt (2015); hbc+07: Honma et al. (2007); hh14: Hou & Han (2014); irm+13: Immer et al. (2013); mdf+11: Moisés et al. (2011); mrm+09: Moscadelli et al. (2009); okh+10: Oh et al. (2010); rus03: Russeil (2003); rag07: Russeil et al. (2007); rbr+10: Rygl et al. (2010); rbs+12: Rygl et al. (2012); srm+14: Sanna et al. (2014); wsr+14: Wu et al. (2014); xrzm06: Xu et al. (2006); xlr+13: Xu et al. (2013b); zzr+09: Zhang et al. (2009); zrm+13: Zhang et al. (2013); zms+14: Zhang et al. (2014).

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