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Table 5.

78 misclassifications found in the Paladini H II region catalogue with the Urumqi λ6 cm data.

P number G-NAME GLong GLat Ref. EB S21 cm EB S11 cm Urumqi S6 cm SRef Freq Ref. Notes
(°) (°) (Jy) (Jy) (Jy) (Jy) (GHz)
130 G10.1+0.7 10.091 0.727 G70 0.7 2.7 G70 NGC 6537, PN (Condon & Kaplan 1998)
0.61 10.0 H87
146 G11.2−0.4 11.172 −0.354 K97 10.367 4.9 K97 SNR G11.2−0.3
11 2.7 A70
11 5.0 A70
8.9 5.0 R70
5.43 10.0 H87
147 G11.2+0.1 11.207 0.088 K97 2.72 2.168 2.529 4.9 K97 SNR G11.1+0.1 (Green 2017)
3.20 4.9 A78 or SNR G11.18+0.11 (Brogan et al. 2006)
157 G11.9+2.2 11.914 2.200 A70 1.74 0.92 0.404 1 1.4 A70 α = −1.22 ± 0.09
1 2.7 A70
162 G12.4+3.8 12.434 3.836 A70 4.80 2.40 1.281 4 1.4 A70 α = −1.08 ± 0.09
198 G15.0−1.6 15.041 −1.569 A70 5 1.4 A70 SNR G15.1−1.6
6 2.7 A70

Notes. Columns 1 and 2: sequential number in the Paladini catalogue and G-names for sources. Columns 3–5: Galactic coordinates and their references. Columns 6–8: flux densities measured from the Effelsberg λ21 cm, λ11 cm and the Urumqi λ6 cm data if available. Columns 9–11: flux density at the corresponding frequency and their reference according to Paladini et al. (2003). The flux densities are reviewed by comparing with those in the original literature. Column 12: remarks why these sources are not considered to be H II regions in this work. Some other references in the 12th column: e.g. Helfand et al. (1989) for P369; Vollmer et al. (2010) for P863. Full table is accessible from the CDS.

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