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Fig. 6

image

From top to bottom: evolutions of the model flux in the 3–10 keV, 10–20 keV, and 20–50 keV ranges (yellow, crimson, and blue points, respectively) using RXTE/PCA, the flux density S14.5 GHz at 14.5 GHz (UMRAO), the BMC normalization and Γ during the 1999 flare transition (R3, R5). Blue vertical strips indicate the phases, when X-ray flux (E> 3 keV) anticorrelates with Γ and the normalization NBMC.

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