Table 5.
Box widths (W) used for box integration, radio beam FWHM converted to physical scales, assumed flux tube radius (R0) used for CR transport modelling for each galaxy; SFR, SFR surface density, and average equipartition magnetic field strength in the galactic disk for individual stripes; gravitational pull for central and outer stripes (as we assume the gravitational potential to be symmetric, there is no distinction for left and right stripes).
| Galaxy | W | Beam | R0 | SFR | ΣSFR | B-Field Strength | Gravitational pull | |||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| [″] | [kpc] | [kpc] | [M⊙ yr–1] |
[M⊙ yr–1 kpc–2]×10−3 |
[μ G] |
[N]×10−10 |
||||||||
| left | middle | right | left | middle | right | left | middle | right | middle | outer | ||||
| NGC 891 | 177 | 0.88 | 7.8 | 0.5 | 1.0 | 0.4 | 3.9 | 5.6 | 2.8 | 9.2 | 13.1 | 9.0 | 3.7 | 0.6 |
| NGC 3432 | 102 | 0.91 | 4.6 | 0.2 | 0.3 | 0.1 | 3.7 | 4.2 | 1.1 | 8.6 | 10.2 | 6.7 | 1.6 | 0.3 |
| NGC 4013 | 63 | 1.36 | 4.3 | 0.2 | 0.3 | 0.1 | 4.6 | 5.6 | 3.8 | 7.5 | 9.1 | 7.3 | 5.0 | 0.8 |
| NGC 4157 | 120 | 1.51 | 9.0 | 0.2 | 1.3 | 0.2 | 1.3 | 5.5 | 1.2 | 8.1 | 13.1 | 7.4 | 2.5 | 0.4 |
| NGC 4631 | 266 | 0.72 | 9.6 | 0.3 | 1.6 | 0.5 | 1.8 | 6.1 | 2.8 | 7.5 | 11.7 | 8.9 | 1.3 | 0.2 |
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