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Electromagnetic radiation initiated by hadronic jets from microquasars in the ISM

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arxiv astro-ph/0411508 v1 pith:ZYH2XCQW submitted 2004-11-17 astro-ph

V. Bosch-Ramon (1) , F. A. Aharonian (2) , J. M. Paredes (1) This is my paper · ORCID
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keywords emissionenergygalactichigh-energymicroquasarspion-decayproduceproduced
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Microquasars are potential candidates to produce a non-negligible fraction of the observed galactic cosmic rays. The protons accelerated at the jet termination shock interact with the interstellar medium and may produce detectable fluxes of extended emission at different energy bands: high-energy and very high-energy gamma-rays produced by neutral pion-decay, synchrotron and bremsstrahlung emission in a wide energy range generated by the secondary electrons produced by charged pion-decay. We discuss the association between this scenario and some of the unidentified EGRET sources in the galactic plane.

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Cited by 3 Pith papers

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

  1. PeV particle acceleration and non-thermal emission in the `minimalist' model of the extended jets in W50/SS433

    astro-ph.GA 2025-09 conditional novelty 6.0 of 10

    A model of SS433/W50's extended jets with diffusive shock acceleration reproduces X-ray spectra, gamma-ray emission, and >20% X-ray polarization, with >10% of jet power going into PeV protons.

  2. Temporal evolution of the periodic GeV signal from 4FGL J1913.2+0512 and analysis of the SS 433 / W50 lobes

    astro-ph.HE 2026-05 conditional novelty 5.0 of 10

    Fermi LAT data analysis detects a time-evolving ~162-day periodic GeV signal from 4FGL J1913.2+0512 linked to SS 433, prominent in 2008-2018 but diminished afterward, indicating multi-year evolution in gamma-ray produ...

  3. SKAO and Gamma-Ray Synergies

    astro-ph.HE 2026-06 unverdicted novelty 2.0 of 10

    Overview of synergies between SKA radio observations and gamma-ray facilities for studying transient, variable, and steady GeV-TeV sources.

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