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Fig. 3

image

Spectra, in the ννLν representation, produced by a power law distribution of particles accounting for a luminosity of 1043 erg s−1 at 1 GHz. The adopted slope is n = 2.5. The solid lines show spectra produced by protons; the dashed lines represent the spectra produced by leptons. The different slopes are due to the different a value, controlling the amount of collimation of the radiation, and not to a differentslope of the electron distribution. The top panel gives examples for ρ = 106 cm. The bottom panel shows examples for ρ = 107 cm. Parameters, listed in Table 1, were found to minimize the required total energy. N0 indicated in units of cm−3 and ρ in cm.

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