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|
|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|
|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|
|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|
|135||G10.3−0.1||10.307||−0.145||R70||14.61||13.77||15.923||20||2.7||A70||Same as P134|
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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