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Table 8
Minimum frequency, νmin, as a function of γmin for the secondary (LHS1) and primary (LHS2) hotspots in the western lobe of Cygnus A.
| LHS1 | LHS2 | |
| γmin | νmin (MHz) | νmin (MHz) |
|
|
||
| 1 | 1.51 × 10-3 | 1.27 × 10-3 |
| 10 | 0.11 | 0.10 |
| 100 | 7.61 | 7.36 |
| 1000 | 540.3 | 559.8 |
| 10 000 | 38.35 × 103 | 42.55 × 103 |
Notes. We used the magnetic field strengths from the 8 GHz background corrected fluxes using the best fitting spectral slope as given in Table 5.
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