Table 1
Continuum sources.
| Source ID | Glon [°] | Glat [°] | Tcont [K] | Type | L.o.s. | Absorption |
|---|---|---|---|---|---|---|
| G43.921-0.479 | 43.92 | −0.48 | 304 | extragal. | ✓ | ✓ |
| G43.890-0.783 | 43.89 | −0.78 | 481 | H II | ✗ | ✗ |
| G43.738-0.620 | 43.74 | −0.62 | 503 | extragal. | ✓ | ✓ |
| G43.177-0.519 | 43.18 | −0.52 | 296 | H II | ✓ | ✗ |
| G42.434-0.260 | 42.43 | −0.26 | 277 | H II | ✗ | ✗ |
| G42.028-0.605 | 42.03 | −0.60 | 519 | extragal. | ✗ | ✗ |
| G41.513-0.141 | 41.51 | −0.14 | 205 | H II | ✗ | ✗ |
Notes. Column 1 gives the source name as listed in the continuum catalog by Wang et al. (2018). Columns 2 and 3 are the Galactic longitude and latitude, respectively. Column 4 denotes the average brightness temperature of the continuum source over an area of 16′′ × 16′′. Column 5 describes the physical nature of the continuum source. Column 6 marks if the continuum source is located along the line of sight (L.o.s), that is within the contour at 4.2 M⊙ pc−2 (see Sect. 3.3). Column 7 indicates ifabsorption above 3σ is detected in the velocity range of Maggie.
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