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A new population of very high energy gamma-ray sources in the Milky Way

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arxiv astro-ph/0504380 v1 pith:ZVJJARFK submitted 2005-04-18 astro-ph

F.A. Aharonian (for the H.E.S.S. Collaboration) This is my paper · ORCID
classification astro-ph
keywords energyhighcosmicsourcesverygamma-raysmilkypopulation
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Very high energy gamma-rays probe the long-standing mystery of the origin of cosmic rays. Produced in the interactions of accelerated particles in astrophysical objects, they can be used to image cosmic particle accelerators. A first sensitive survey of the inner part of the Milky Way with the High Energy Stereoscopic System (H.E.S.S.) reveals a population of eight previously unknown firmly detected sources of very high energy gamma-rays. At least two have no known radio or X-ray counterpart and may be representative of a new class of `dark' nucleonic cosmic ray sources.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 287 citations worldwide. Full citation record

  1. Multiwavelength study of non-thermal emission in the Swift J1834.9-0846/W41 region

    astro-ph.HE 2026-07 conditional novelty 5.0 of 10

    Modeling favors a lepto-hadronic supernova remnant for the extended TeV emission from HESS J1834-087 plus a leptonic magnetar wind nebula for the central point-like source, with an implied magnetar birth spin period b...

  2. Non-thermal emission from the vicinity of the magnetar CXOU J171405.7-381031

    astro-ph.HE 2026-07 conditional novelty 4.0 of 10

    Both leptonic and lepto-hadronic models fit the CTB 37B gamma-ray spectrum; neutral-pion decay matches above ~10 TeV but needs ~10^51 erg in protons unless the remnant hits dense gas.

  3. Constraining leptonic and hadronic gamma-ray emission from HESS J1825-137 and its environment

    astro-ph.HE 2026-06 unverdicted novelty 4.0 of 10

    Multi-telescope spectral modeling of HESS J1825-137 using Naima and MCMC shows leptonic dominance for existing GeV-TeV data but lepto-hadronic preference when adding simulated CTAO or LHAASO UHE points.

  4. Introduction to multi-messenger astronomy

    astro-ph.HE 2019-07 unverdicted

    The paper supplies an introductory lecture-style summary of observational techniques, astronomical sources, and physical processes across the four main messengers in multi-messenger astronomy.

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