Table 4
GLOSTAR D-configuration sources that are detected as fragmented sources (e.g., multiple components or over-resolved of an extended source) in the B-configuration images.
| GLOSTAR B-conf. | GLOSTAR D-conf. | Num. | Sint | Class |
|---|---|---|---|---|
| Gname | Gname | frags. | (mJy) | |
| (1) | (2) | (3) | (4) | |
| G003.3511-00.0774 | G003.350-00.077 | 3 | 100.98 | HII |
| G005.4751-00.2430 | G005.476-00.244 | 3 | 15.32 | HII |
| G008.1397-00.0271 | G008.140-00.027 | 2 | 4.88 | HII |
| G008.6693-00.3560 | G008.669-00.356 | 3 | 231.16 | HII |
| ⋮ | ⋮ | ⋮ | ⋮ | ⋮ |
| G027.1858-00.0817 | G027.186-00.081 | 2 | 7.76 | HII |
| G027.2799+00.1446 | G027.280+00.144 | 4 | 51.44 | HII |
| G027.7018+00.7040 | G027.701+00.705 | 2 | 6.98 | PN |
| G038.8757+00.3080 | G038.876+00.308 | 2 | 52.67 | HII |
| G056.6162+00.1707 | G056.616+00.171 | 3 | 11.25 | Egc |
Notes. Column 1 shows the GLOSTAR B-configuration name of the brightest member in the clusters. Column 2 shows the GLOSTAR D-configuration name for the over-resolved/ſragmenColumnsted clusters, as shown in the middle panel of Fig. 9. Columns 3 and 4 show the number of fragments and the integrated fluxes of the brightest component. Column 5 shows the source type as classified in Sect. 3.6. Other properties can be found in Table 3. Only a small portion of the data is provided here. The full table is available at the CDS.
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