Table 1
Properties of PHANGS-MUSE galaxies used in this work.
| Name | Parent number | SNRs number | Distance (Mpc) | Plate scale pc/″ | log(M*) (M⊙) | log(SFR) (M⊙yr−1) | PA (deg) | i (deg) | Survey Area (kpc2) |
|---|---|---|---|---|---|---|---|---|---|
| IC 5332 | 36 | 24 | 9.0 | 43.7 | 9.68 | −0.39 | 74.4 | 26.9 | 34 |
| NGC 628 | 120 | 79 | 9.8 | 47.7 | 10.34 | 0.24 | 20.7 | 8.9 | 89 |
| NGC 1087 | 123 | 29 | 15.9 | 76.8 | 9.94 | 0.11 | 359.1 | 42.9 | 126 |
| NGC 1300 | 23 | 15 | 19.0 | 92.1 | 10.62 | 0.07 | 278.0 | 31.8 | 356 |
| NGC 1365 | 63 | 38 | 19.6 | 94.9 | 11.00 | 1.24 | 201.1 | 55.4 | 409 |
| NGC 1385 | 114 | 63 | 17.2 | 83.5 | 9.98 | 0.32 | 181.3 | 44.0 | 101 |
| NGC 1433 | 46 | 24 | 18.6 | 90.3 | 10.87 | 0.05 | 199.7 | 28.6 | 426 |
| NGC 1512 | 25 | 20 | 18.8 | 91.3 | 10.72 | 0.11 | 261.9 | 42.5 | 266 |
| NGC 1566 | 180 | 101 | 17.7 | 85.8 | 10.79 | 0.66 | 214.7 | 29.5 | 208 |
| NGC 1672 | 61 | 28 | 19.4 | 94.1 | 10.73 | 0.88 | 134.3 | 42.6 | 250 |
| NGC 2835 | 187 | 119 | 12.2 | 59.2 | 10.00 | 0.10 | 1.0 | 41.3 | 87 |
| NGC 3351 | 46 | 24 | 10.0 | 48.3 | 10.37 | 0.12 | 193.2 | 45.1 | 73 |
| NGC 3627 | 152 | 86 | 11.3 | 54.9 | 10.84 | 0.59 | 173.1 | 57.3 | 85 |
| NGC 4254 | 332 | 154 | 13.1 | 63.5 | 10.42 | 0.49 | 68.1 | 34.4 | 169 |
| NGC 4303 | 303 | 130 | 17.0 | 82.4 | 10.51 | 0.73 | 312.4 | 23.5 | 214 |
| NGC 4321 | 132 | 80 | 15.2 | 73.7 | 10.75 | 0.55 | 156.2 | 38.5 | 191 |
| NGC 4535 | 75 | 54 | 15.8 | 76.5 | 10.54 | 0.34 | 179.7 | 44.7 | 124 |
| NGC 5068 | 194 | 92 | 5.2 | 25.2 | 9.41 | −0.56 | 342.4 | 35.7 | 23 |
| NGC 7496 | 21 | 6 | 18.7 | 90.8 | 10.00 | 0.35 | 193.7 | 35.9 | 92 |
Notes. For Cols. parent and SNRs, see Sect. 3.1.4 for their detailed classification. Distances of PHANGS galaxies come from Anand et al. (2021), with a complete set of references provided in the acknowledgments. Their stellar masses and star formation rates (SFRs) are from Leroy et al. (2021). Position angle (PA) and inclination (i) come from the CO (2–1) dynamics of PHANGS-ALMA (Lang et al. 2020). Survey areas are using the values from Belfiore et al. (2022).
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