Disentangling multiple gas kinematic drivers in the Perseus galaxy cluster

Marc Audard; Hisamitsu Awaki; Ralf Ballhausen; Bamba Aya; E. Behar; Rozenn Boissay-Malaquin; Laura Brenneman; V. Brown; Lía Corrales; P. Coppi; Renata Cumbee; María Díaz Trigo; C Done; Tadayasu Dotani; Ken Ebisawa; M. J. Eckart; Dominique Eckert; Satoshi Eguchi; Teruaki Enoto; Yuichiro Ezoe; Adam Foster; Ryuichi Fujimoto; Yutaka Fujita; Kento Torigoe; Kotaro Fukushima; Akihiro Furuzawa; Luigi Gallo; S. Gunji; Liyi Gu; P. J. Serlemitsos; Kouichi Hagino; Kenji Hamaguchi; I. Harrus; Katsuhiro Hayashi; Takayuki Hayashi; Natalie Hell; Edmund Hodges‐Kluck; A. Ptak; Yuto Ichinohe; Daiki Ishi; Manabu Ishida; Aya Kubota; Yoshitaka Ishisaki; J. S. Kaastra; Timothy Kallman; Erin Kara; Satoru Katsuda; Yoshiaki Kanemaru; Richard Kelley; Caroline Kilbourne; Shunji Kitamoto; Shogo Kobayashi; Takayoshi Kohmura; Aya Kubota; Maurice Leutenegger; Michael Loewenstein; Y. Maeda; Maxim Markevitch; Hironori Matsumoto; Kyoko Matsushita; Dan McCammon; Brian McNamara; François Mernier; Mike McDonald; R. C. Reis; Ikuyuki Mitsuishi; Misaki Mizumoto; T Mizuno; Koji Mori; Koji Mukai; Hiroshi Murakami; S. S. Holt; Hiroshi Nakajima; Kazuhiro Nakazawa; Liming Song; Kumiko Nobukawa; Masayoshi Nobukawa; HIROFUMI NODA; Hirokazu Odaka; Shoji Ogawa; Anna Ogorzalek; Takashi Okajima; Naomi Ota; Stephane Paltani; R. Petre; Paul Plucinsky; Frederick S. Porter; K. Pottschmidt; Kosuke Sato; Toshiki Sato; Makoto Sawada; Hiromi Seta; Megumi Shidatsu; A. Simionescu; Randall Smith; Hiromasa Suzuki; Andrew Szymkowiak; Hiromitsu Takahashi; Mai Takeo; Toru Tamagawa

doi:10.1038/s41586-025-10017-x

January 28, 2026Nature

Disentangling multiple gas kinematic drivers in the Perseus galaxy cluster

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Key Points

Gas kinematics reveals intricacies of gravitational interactions within the Perseus galaxy cluster, enhancing our comprehension of cosmic structures.
Key findings show multiple gas kinematic drivers, demonstrating variability and complexity in motion throughout the cluster.
Observational analysis distinguishes these drivers across different scales, emphasizing the role of both internal and external forces shaping gas dynamics.
Understanding these kinematic drivers highlights the need for further studies to explore their implications on galaxy formation and evolution.

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Implication

Observational analysis uncovers multiple gas kinematic drivers in the Perseus galaxy cluster, suggesting complex interactions at play.

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Audard et al. (2026) studied this question.

synapsesocial.com/papers/69a75c5ac6e9836116a252e9 https://doi.org/10.1038/s41586-025-10017-x

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Disentangling multiple gas kinematic drivers in the Perseus galaxy cluster

Key Points

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Disentangling multiple gas kinematic drivers in the Perseus galaxy cluster

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