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Probable Detection of a Cooler Gas Component in the Perseus Cluster with XRISM

Fuente: arXiv

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Bibliographic Details
Main Authors:	Meunier, Julian, McNamara, Brian R., Simionescu, Aurora, Mernier, François, Zhuravleva, Irina, Zhang, Congyao, Heinrich, Annie, Hlavacek-Larrondo, Julie, Porter, Frederick S., Vigneron, Benjamin, ZuHone, John, Bellomi, Elena, Drury, Ian, Eckart, Megan E., Fujimoto, Ryuichi, Fujita, Yutaka, Gu, Liyi, Hatsukade, Isamu, Ichinohe, Yuto, Kanemaru, Yoshiaki, Kitaguchi, Takao, Kitamoto, Shunji, Kobayashi, Shogo, Kohmura, Takayoshi, Matsumoto, Hironori, Matsushita, Kyoko, Migkas, Kostas, Mitsuishi, Ikuyuki, Mori, Koji, Nakajima, Hiroshi, Noda, Hirofumi, Ogorzalek, Anna, Ota, Naomi, Shefler, Lior, Truong, Nhut, Tümer, Ayşegül, Uchida, Nagomi, Uchida, Yuusuke, Ueda, Shutaro
Format:	Preprint
Published:	2026
Subjects:	High Energy Astrophysical Phenomena Astrophysics of Galaxies
Online Access:	Acceder al recurso
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