Table D.6.
Diffusion models with an energy-dependent diffusion coefficient for NGC 4565 (μ = 0.5).
| r [kpc] | D0 [1028 cm2 s−1] | B0 [μG] | hB2 [kpc] | hB2/hB2, eq |
 |
|---|---|---|---|---|---|
| −13.85 N |
 |
5.5 |
 |
1.96 | 0.40 |
| −13.85 S |
 |
5.5 |
 |
1.96 | 0.48 |
| −6.92 N |
 |
6.4 |
 |
3.70 | 1.43 |
| −6.92 S |
 |
6.4 |
 |
3.70 | 1.25 |
| 0 N |
 |
6.3 |
 |
3.00 | 0.32 |
| 0 S |
 |
6.3 |
 |
3.00 | 0.59 |
| 6.92 N |
 |
6.5 |
 |
3.21 | 0.22 |
| 6.92 S |
 |
6.5 |
 |
3.02 | 0.83 |
| 13.85 N |
 |
5.2 |
 |
3.73 | 0.49 |
| 13.85 S |
 |
5.2 |
 |
3.73 | 0.72 |
Notes. “N” denotes north of the mid-plane, “S” denotes south of the mid-plane; D0: diffusion coefficient [D(E) = D0(E/1 GeV)μ]; B0: mid-plane magnetic field strength; hB1: scale height of the disc magnetic field; hB2: scale height of the halo magnetic field; hB1, eq, hB2, eq: scale height of the disc or halo magnetic field if energy equipartition is assumed; 
: reduced χ2 of the fit to the intensity profile; 
: reduced χ2 of the fit to the spectral index profile.
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