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Neutrinos and gamma rays from Seyfert galaxies constrain the properties of coronal turbulence

Fuente: arXiv

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Détails bibliographiques
Auteurs principaux:	Testagrossa, Federico, Fiorillo, Damiano F. G., Comisso, Luca, Peretti, Enrico, Petropoulou, Maria, Sironi, Lorenzo
Format:	Preprint
Publié:	2026
Sujets:	High Energy Astrophysical Phenomena High Energy Physics - Phenomenology
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

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