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XRISM reveals low non-thermal pressure in the core of the hot, relaxed galaxy cluster Abell 2029

Fuente: arXiv

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Détails bibliographiques
Auteur principal:	XRISM Collaboration
Format:	Preprint
Publié:	2025
Sujets:	High Energy Astrophysical Phenomena
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

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