Table 1
Completeness of each evolutionary class.
H ii | SFCs | SLCs | No class | ||
|
|||||
Total | 114 | 184 | 210 | 107 | |
Known da | 84 | 126 | 120 | – | |
d < 5.5 kpc | 57 | 99 | 111 | – | |
d > 5.5 kpc | 27 | 27 | 9 | – | |
miss. d < 5.5 kpcb | 20 | 18 | 102 | 87 | |
miss. d > 5.5 kpcb | 10 | 8 | 8 | 20 | |
Studied | 57 | 99 | 31c | – |
Notes.
Only SLCs with KDA solved and, if more than one distance estimate, agreement between different literature sources.
Number of regions lost due to lack of distance estimates. We assume homogeneous distribution of the sources along the Galactic plane area studied.
We only studied isolated SLCs (see Sect. 2.2).
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