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Table 3
Ionising photon budget for entire galaxies.
| H II regions | Stellar associations | Star cluster | |||
|---|---|---|---|---|---|
| Name | log(QHα/s−1) | log (Q(H0)/s−1 | fesc (%) | log(Q(H0)/s−1) | fesc (%) |
| IC 5332 | 51.56 ± 0.06 | 52.38 ± 0.04 | 84.9 ± 2.5 | 52.13 ± 0.36 | 73.0 ± 22.5 |
| NGC 0628 | 52.50 ± 0.04 | 53.29 ± 0.01 | 83.5 ± 1.6 | 53.05 ± 0.58 | 71.7 ± 37.7 |
| NGC 1087 | 53.11 ± 0.06 | 53.65 ± 0.04 | 71.4 ± 4.6 | 53.55 ± 0.15 | 63.7 ± 13.0 |
| NGC 1300 | 52.70 ± 0.04 | 52.97 ± 0.06 | 45.5 ± 9.2 | 53.25 ± 1.98 | 71.5 ± 130.1 |
| NGC 1365 | 53.15 ± 0.14 | 53.43 ± 0.06 | 47.5 ± 18.4 | 53.48 ± 0.57 | 52.8 ± 64.0 |
| NGC 1385 | 53.34 ± 0.05 | 53.70 ± 0.04 | 56.3 ± 6.4 | 53.61 ± 0.04 | 46.8 ± 7.3 |
| NGC 1433 | 52.26 ± 0.04 | 52.71 ± 0.02 | 64.0 ± 4.0 | 53.00 ± 0.14 | 81.4 ± 7.1 |
| NGC 1512 | 52.29 ± 0.05 | 52.62 ± 0.03 | 53.2 ± 6.3 | 53.59 ± 0.17 | 95.0 ± 5.6 |
| NGC 1566 | 53.44 ± 0.06 | 53.99 ± 0.02 | 71.7 ± 4.0 | 53.85 ± 0.20 | 61.4 ± 17.8 |
| NGC 1672 | 53.26 ± 0.05 | 53.72 ± 0.02 | 65.5 ± 4.1 | 53.67 ± 0.42 | 61.1 ± 37.4 |
| NGC 2835 | 52.56 ± 0.05 | 53.14 ± 0.03 | 74.1 ± 3.6 | 53.18 ± 0.44 | 76.1 ± 24.2 |
| NGC 3351 | 51.99 ± 0.04 | 52.95 ± 0.05 | 89.0 ± 1.6 | 52.72 ± 0.19 | 81.5 ± 8.3 |
| NGC 3627 | 53.42 ± 0.04 | 53.75 ± 0.05 | 53.9 ± 7.0 | 53.81 ± 0.29 | 59.7 ± 27.5 |
| NGC 4254 | 53.47 ± 0.02 | 54.06 ± 0.03 | 74.1 ± 2.2 | 54.10 ± 0.04 | 76.6 ± 2.6 |
| NGC 4303 | 53.60 ± 0.03 | 54.13 ± 0.02 | 70.0 ± 2.6 | 54.17 ± 0.07 | 72.9 ± 4.9 |
| NGC 4321 | 53.05 ± 0.04 | 53.77 ± 0.02 | 80.8 ± 2.1 | 53.69 ± 0.05 | 76.9 ± 3.3 |
| NGC 4535 | 52.73 ± 0.04 | 53.27 ± 0.05 | 71.0 ± 4.2 | 53.34 ± 0.16 | 75.4 ± 9.6 |
| NGC 5068 | 52.20 ± 0.05 | 52.63 ± 0.04 | 62.9 ± 5.6 | 52.67 ± 0.12 | 65.7 ± 10.8 |
| NGC 7496 | 52.62 ± 0.06 | 53.23 ± 0.03 | 75.8 ± 3.9 | 53.20 ± 0.05 | 74.0 ± 4.7 |
| Total | 54.36 ± 0.02 | 54.87 ± 0.01 | 68.9 ± 1.3 | 54.88 ± 0.07 | 69.6 ± 5.0 |
Notes. We use the H II regions from Santoro et al. (2022) and Groves et al. (2023) and either the stellar associations (32 pc, NUV) from Larson et al. (2023), or the compact star clusters from Thilker et al. (2022).
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