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arxiv: 1501.00973 · v2 · pith:X3UP2AQXnew · submitted 2015-01-05 · 🌌 astro-ph.HE

Multi-TeV flaring from blazars: Markarian 421 a case study

classification 🌌 astro-ph.HE
keywords flaringmulti-tevblazarenergiesenergymarkarianmodelobserved
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The TeV blazar Markarian 421 underwent multi-TeV flaring during April 2004 and simultaneously observed in x-ray and TeV energies. It was observed that the TeV outbursts had no counterparts in the lower energies, which implies that this might be an orphan flare. In the context of hadronic model, we have shown that this multi-TeV flaring can be produced due to the interaction of Fermi-accelerated protons of energy $\lesssim 168$ TeV with the background photons in the low energy tail of the synchrotron self-Compton spectrum of the blazar jet. We fit very well the flaring spectrum with this model. Based on this study, we speculate that Mrk 501 and PG 1553+113 are possible candidates for orphan flaring in the future.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Multi-TeV flaring in nearby High Energy Blazars: A photohadronic scenario

    astro-ph.HE 2019-07 unverdicted novelty 2.0

    Review applies the photohadronic model with EBL corrections to explain multi-TeV flaring in three nearby blazars.