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Delayed Radio Flares in Neutrino-associated Blazars: The Case of TXS 0506+056

  • Authors: S. I. Stathopoulos, C. Yuan, G. Vasilopoulos, F. Testagrossa, D. Karavola, M. Petropoulou, W. Winter

S. I. Stathopoulos et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 4.

Multifrequency RATAN-600 radio light curves of TXS 0506+056 at 1.2–22 GHz (markers with 1σ uncertainties), shown with vertical offsets of 2 Jy between adjacent bands for clarity. The solid curves correspond to Scenario C (redissipation followed by jet deceleration). The vertical dashed line marks the onset of the deceleration phase, after which the Doppler factor is assumed to decrease as a power law. For each band, the thin horizontal dashed line indicates the estimated quiescent/background level.

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