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Table 3.
CRe transport length and spectral indices of the RPS sample.
| Name |
 |
 |
 |
|---|---|---|---|
| [kpc] | [kpc] | ||
| IC 3105 | – | 2.3 | < − 0.36 (a) |
| NGC 4254 | 5.2 | 5.4 | −0.77 ± 0.10 (b) |
| NGC 4302 | 4.4 | 3.9 | −0.77 ± 0.10 (c) |
| NGC 4330 | 1.9 | 1.1 | −0.63 ± 0.11 (c) |
| IC 3258 | – | 1.8 | < − 0.74 (a) |
| NGC 4396 | 2.3 | 1.3 | −0.79 ± 0.10 (c) |
| NGC 4402 | 1.4 | 1.6 | −0.81 ± 0.10 (c) |
| NGC 4424 | 1.9 | 1.4 | −0.67 ± 0.11 (c) |
| NGC 4501 | 1.3 | 0.9 | −0.75 ± 0.10 (c) |
| IC 3476 | 1.7 | 1.8 | −0.81 ± 0.1 (a) |
| NGC 4522 | 1.0 | 1.6 | −0.48 ± 0.10 (b) |
| IC 800 | – | 2.2 | < − 0.76 (a) |
| NGC 4548 | – | 5.5 | −1.32 ± 0.10 (d) |
| NGC 4569 | 2.5 | 2.0 | −0.55 ± 0.10 (b) |
| NGC 4607 | 1.6 | 1.5 | −0.70 ± 0.10 (d) |
| NGC 4634 | 2.0 | 1.8 | −0.66 ± 0.10 (e) |
| NGC 4654 | 3.0 | 3.0 | −0.87 ± 0.10 (d) |
Notes. The 1.4 GHz flux densities for the spectral index estimation are taken from:
(a)
NVSS (4σ upper limits Condon et al. 1998);
(d)
measured from the maps provided by Chung et al. (2009) and
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