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arxiv: 2505.06533 · v1 · pith:K7OTO3JWnew · submitted 2025-05-10 · 🌌 astro-ph.CO · astro-ph.HE

Constraining gas motion and non-thermal pressure beyond the core of the Abell 2029 galaxy cluster with XRISM

XRISM Collaboration: Marc Audard , Hisamitsu Awaki , Ralf Ballhausen , Aya Bamba , Ehud Behar , Rozenn Boissay-Malaquin , Laura Brenneman , Gregory Brown
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Lia Corrales Elisa Costantini Renata Cumbee Maria Diaz Trigo Chris Done Tadayasu Dotani Ken Ebisawa Megan Eckart Dominique Eckert Satoshi Eguchi Teruaki Enoto Yuichiro Ezoe Adam Foster Ryuichi Fujimoto Yutaka Fujita Yasushi Fukazawa Kotaro Fukushima Akihiro Furuzawa Luigi Gallo Javier Garc\'ia Liyi Gu Matteo Guainazzi Kouichi Hagino Kenji Hamaguchi Isamu Hatsukade Katsuhiro Hayashi Takayuki Hayashi Natalie Hell Edmund Hodges-Kluck Ann Hornschemeier Yuto Ichinohe Daiki Ishi Manabu Ishida Kumi Ishikawa Yoshitaka Ishisaki Jelle 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 Yoshitomo Maeda Maxim Markevitch Hironori Matsumoto Kyoko Matsushita Dan McCammon Brian McNamara Francois Mernier Eric Miller Jon Miller Ikuyuki Mitsuishi Misaki Mizumoto Tsunefumi Mizuno Koji Mori Koji Mukai Hiroshi Murakami Richard Mushotzky Hiroshi Nakajima Kazuhiro Nakazawa Jan-Uwe Ness Kumiko Nobukawa Masayoshi Nobukawa Hirofumi Noda Hirokazu Odaka Shoji Ogawa Anna Ogorzalek Takashi Okajima Naomi Ota Stephane Paltani Robert Petre Paul Plucinsky Frederick Porter Katja Pottschmidt Kosuke Sato Toshiki Sato Makoto Sawada Hiromi Seta Megumi Shidatsu Aurora Simionescu Randall Smith Hiromasa Suzuki Andrew Szymkowiak Hiromitsu Takahashi Mai Takeo Toru Tamagawa Keisuke Tamura Takaaki Tanaka Atsushi Tanimoto Makoto Tashiro Yukikatsu Terada Yuichi Terashima Yohko Tsuboi Masahiro Tsujimoto Hiroshi Tsunemi Takeshi Tsuru Hiroyuki Uchida Nagomi Uchida Yuusuke Uchida Hideki Uchiyama Yoshihiro Ueda Shinichiro Uno Jacco Vink Shin Watanabe Brian J. Williams Satoshi Yamada Shinya Yamada Hiroya Yamaguchi Kazutaka Yamaoka Noriko Yamasaki Makoto Yamauchi Shigeo Yamauchi Tahir Yaqoob Tomokage Yoneyama Tessei Yoshida Mihoko Yukita Irina Zhuravleva Tommaso Bartalesi Stefano Ettori Roman Kosarzycki Lorenzo Lovisari Tom Rose Arnab Sarkar Ming Sun Prathamesh Tamhane
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classification 🌌 astro-ph.CO astro-ph.HE
keywords pressureabellclustercorehydrostaticnon-thermalbeyondbias
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We report a detailed spectroscopic study of the gas dynamics and hydrostatic mass bias of the galaxy cluster Abell 2029, utilizing high-resolution observations from XRISM Resolve. Abell 2029, known for its cool core and relaxed X-ray morphology, provides an excellent opportunity to investigate the influence of gas motions beyond the central region. Expanding upon prior studies that revealed low turbulence and bulk motions within the core, our analysis covers regions out to the scale radius $R_{2500}$ (670~kpc) based on three radial pointings extending from the cluster center toward the northern side. We obtain accurate measurements of bulk and turbulent velocities along the line of sight. The results indicate that non-thermal pressure accounts for no more than 2% of the total pressure at all radii, with a gradual decrease outward. The observed radial trend differs from many numerical simulations, which often predict an increase in non-thermal pressure fraction at larger radii. These findings suggest that deviations from hydrostatic equilibrium are small, leading to a hydrostatic mass bias of around 2% across the observed area.

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