Minimum frequency, νmin, as a function of γmin for the secondary (LHS1) and primary (LHS2) hotspots in the western lobe of Cygnus A.
|γmin||νmin (MHz)||νmin (MHz)|
|1||1.51 × 10-3||1.27 × 10-3|
|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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