Fig. 9.

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Flares at different wavelengths. (a) Flare in a self-absorbed region. The parameters have the following values: cm,
G,
erg s−1,
, uexp = 0.1 c, γmin = 1, γmax = 106, p = 2, δ = 10, and z0 = 0.001 pc. The magnetic field decreases as B′∝R′ − 1 and the electron luminosity as
. For the γ-ray flare, we used a pulse which was injected at
, with a width w′ = 50 tcross, 0 and α = 45. The dashed lines represent the emission of the blob without the reaccelerating episode; (b) flare in an optically thin region. In this case, we change only the initial electron luminosity
erg s−1 and the reaccelerating episode occurs at the time,
, the rest of the parameters are the same as in case (a).
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