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Hadronic gamma-ray emission from windy microquasars

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arxiv astro-ph/0309123 v1 pith:EMUXCJUB submitted 2003-09-04 astro-ph

Gustavo E. Romero , Diego F. Torres , M. M. Kaufman Bernado , I. F. Mirabel This is my paper · ORCID
classification astro-ph
keywords gamma-rayemissionhadronicmicroquasarsstellarcompanionsdensedetectability
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The jets of microquasars with high-mass stellar companions are exposed to the dense matter field of the stellar wind. We present estimates of the gamma-ray emission expected from the jet-wind hadronic interaction and we discuss the detectability of the phenomenon at high energies. The proposed mechanism could explain some of the unidentified gamma-ray sources detected by EGRET instrument on the galactic plane.

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Cited by 2 Pith papers

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

  1. 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...

  2. uGMRT observation of the unidentified PeVatron candidate LHAASO J2108+5157

    astro-ph.HE 2024-12 reject novelty 5.0 of 10

    A new 650 MHz uGMRT image reveals an extended disk-jet radio source inside the LHAASO J2108+5157 error circle, proposed as a microquasar counterpart to the PeVatron.

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