Table 1.
Properties of galaxies in the sample.
| Galaxy | d | r⋆ | ΣSFR | Beq | p | v | i | SFR |
|---|---|---|---|---|---|---|---|---|
| (Mpc) | (kpc) | ( ) |
(μG) | (%) |
 |
(° ) | (M⊙ yr−1) | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| NGC 0628 | 7.2 | 11.5 | 2.8 × 10−3 | 9.0 | 11.50 | 217 | 7 | 1.19 |
| NGC 0925 | 9.1 | 14.9 | 1.1 × 10−3 | 6.2 | 0.67 | 136 | 66 | 0.75 |
| NGC 2403 | 3.06 | 8.0 | 4.5 × 10−3 | 7.5 | 7.78 | 134 | 63 | 0.90 |
| NGC 2841 | 14.1 | 16.0 | 2.3 × 10−3 | 6.4 | 5.80 | 302 | 74 | 1.88 |
| NGC 2903 | 8.9 | 13.2 | 1.1 × 10−2 | 11.0 | 3.04 | 190 | 66 | 5.96 |
| NGC 2976 | 3.55 | 3.1 | 3.9 × 10−3 | 8.3 | 4.41 | 92 | 54 | 0.12 |
| NGC 3184 | 11.7 | 14.0 | 2.4 × 10−3 | 7.5 | 6.25 | 210 | 16 | 1.49 |
| NGC 3198 | 14.1 | 14.0 | 2.4 × 10−3 | 6.0 | 1.02 | 150 | 72 | 1.49 |
| NGC 3938 | 17.9 | 15.6 | 3.9 × 10−3 | 8.9 | 7.75 | 128 | 36 | 2.98 |
| NGC 4254 | 14.4 | 10.5 | 1.7 × 10−2 | 16.0 | 4.71 | 300 | 33 | 5.94 |
| NGC 4725 | 11.9 | 13.2 | 2.2 × 10−3 | 6.5 | 3.60 | 257 | 43 | 1.19 |
| NGC 4736 | 4.66 | 4.9 | 1.2 × 10−2 | 12.1 | 3.59 | 156 | 41 | 0.94 |
| NGC 5055 | 7.94 | 15.2 | 5.9 × 10−3 | 9.1 | 3.89 | 192 | 59 | 2.98 |
| NGC 5194 | 8.0 | 16.0 | 1.5 × 10−2 | 12.0 | 5.70 | 219 | 20 | 11.89 |
| NGC 7331 | 14.5 | 22.8 | 4.6 × 10−3 | 8.0 | 2.45 | 244 | 77 | 7.48 |
Notes. Column 2: d is the distance (Heesen et al. 2022); (3) r⋆ is the star formation radius as obtained from radio continuum (Heesen et al. 2022); (4) is the SFR surface density within r⋆; (5) Beq is the total magnetic field strength estimated from energy equipartition (Chyży et al. 2007; Mulcahy et al. 2017; Heesen et al. 2023b, for NGC 2903 we use the B–ΣSFR relation); (6) p is the polarisation fraction at 1365 MHz (Heald et al. 2009); (7) v is the rotation velocity of the galaxy (Heesen et al. 2022); (8) i is the inclination angle (Heesen et al. 2022); and (9) SFR is the integrated star formation rate (Heesen et al. 2022).
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