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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 3.

Profiles of the comoving nonthermal electron/positron number density ﹩{n}_{{\rm{e}}}^{{\prime} }﹩ (left axis, solid black line) together with the Doppler factor ﹩\delta ({R}^{{\prime} })﹩ (right axis, blue dashed line) as a function of the radius of the emitting region ﹩{R}^{{\prime} }﹩. The dotted black line shows the asymptotic ﹩{R}^{{\prime} -2}﹩ scaling at large radii. The vertical dashed lines mark the transition to the reacceleration phase at ﹩{t}_{{\rm{reacc}}}^{{\prime} }﹩ and the deceleration time ﹩{t}_{{\rm{dec}}}^{{\prime} }﹩. The shaded regions indicate the expansion and resdissipation phases.

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