Table 2.
Observed properties of the sub-sample of regions shown in Fig. 8 and of the overall H II regions and DIG population.
| Region ID | Stellar content |
tmax | log MGMC | E(B − V) | log L(Hα) | Classification | ||
|---|---|---|---|---|---|---|---|---|
| YSC | O⋆ | WR | [Myr] | [M⊙] | [erg s−1] | |||
| 1 | 24 | 111 | 6 |
 |
6.1 | 0.14 | 39.11 | CH |
| 2 | 3 | 30 | 1 |
 |
6.0 | 0.13 | 38.68 | CH |
| 3 | 4 | 26 | 1 |
 |
5.3 | 0.19 | 38.73 | CH |
| 4 | 1 | 19 | 0 |
 |
4.5 | 0.12 | 38.25 | IB |
| 5 | 0 | 5 | 0 | ≤3.0 | 3.4 | 0.14 | 37.35 | IB |
| 6 | 1 | 2 | 0 |
 |
– | 0.09 | 37.41 | CH |
| 7 | 1 | 2 | 0 |
 |
– | 0.11 | 37.01 | IB |
| 8 | 8 | 110 | 1 |
 |
6.3 | 0.17 | 38.89 | CH |
| Tot H II | 47 | 404 | 8 | |||||
| Tot DIG | 49 | 271 | 1 | |||||
Notes. We note that the number of O stars indicated here is not completeness-corrected. tmax indicates the age of the oldest cluster in each region (fiducial value of 50 ± 25 percentile of the age PDF; masking cluster with ages > 10 Myr). In the case of region 5, which is hosting exclusively O stars, we have assumed 3 Myr as an upper limit for the age. The indicated E(B − V) is the median extinction in the region (estimated from the Balmer decrement). The total L(Hα) in each region is reddening corrected. Regions are classified as described in Sect. 6 into ‘classical’ ionisation bounded regions (IB) and regions featuring optically thin channels (CH).
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