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A $\sim 43$ GeV $γ$-ray line signature in the directions of a group of nearby massive galaxy clusters

Fuente: arXiv

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Détails bibliographiques
Auteurs principaux:	Fan, Yi-Zhong, Shen, Zhao-Qiang, Liang, Yun-Feng, Li, Xiang, Duan, Kai-Kai, Xia, Zi-Qing, Huang, Xiao-Yuan, Feng, Lei, Yuan, Qiang
Format:	Preprint
Publié:	2024
Sujets:	High Energy Astrophysical Phenomena Cosmology and Nongalactic Astrophysics 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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