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| Journal Article | PUBDB-2026-02382 |
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2026
EDP Sciences
Les Ulis
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Please use a persistent id in citations: doi:10.1051/0004-6361/202555824 doi:10.3204/PUBDB-2026-02382
Report No.: arXiv:2603.21912
Abstract: Context. Composite galaxies that contain both Seyfert and starburst components may produce very high-energy (VHE; > 100 GeV) γ-ray emission at a wide range of spatial scales, from a few Schwarzschild radii of a supermassive black hole (SMBH; RS = 10−6 pc for MSMBH = 107 M⊙) to dimensions of kiloparsec-size jet-driven outflows. In addition to supernova remnants, various sources have been suggested to explain data collected on composite galaxies, including multi-messenger neutrino and ultra-high-energy cosmic-ray data.Aims. The closest composite Seyfert–starburst galaxies (NGC 1068, the Circinus galaxy, and NGC 4945) are observed with the High Energy Stereoscopic System (H.E.S.S.) to provide constraints on cosmic-ray populations in these systems.Methods. Data obtained in H.E.S.S. observations have been analyzed to search for VHE γ-ray counterparts to the GeV γ-ray signals detected with Fermi-LAT and for potential spectral components in the VHE range.Results. No significant signals have been found in these H.E.S.S. data. Upper limits on the VHE γ-ray fluxes were applied to constrain theoretical models involving different spectral components.Key words: relativistic processes / ISM: jets and outflows / galaxies: Seyfert / galaxies: starburst / gamma rays: galaxies★★ The authors honor the memory of Sergio Colafrancesco, who brought us together in pursuit of this study during his final years.
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H.E.S.S. observations of composite Seyfert–starburst galaxies
(2026)
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