collaborators

8 papers

astro-ph.CO2026

XRISM-Subaru views of Abell 754: an off-axis, near-line-of-sight merging cluster

Nobuhiro Okabe, Yuki Omiya, Kazuhiro Nakazawa +4

We report a weak-lensing (WL) mass measurement for the merging cluster Abell 754 and impose constraints on the merger trajectory. The trajectory analysis adopts a two-body model wi…

astro-ph.GA2026

Revisiting thermodynamics at the outskirts of the Perseus cluster with Suzaku: importance of modeling the Hot Galactic gas

Kyoko Matsushita, Hayato Sugiyama, Masaki Ueda +5

The thermodynamic properties of the intracluster medium (ICM) at the outskirts of galaxy clusters provide valuable insights into the growth of the dark matter halo and the heating…

astro-ph.GA2025

XRISM-Subaru views of Abell 754: Energetic ICM Motions Revealed by XRISM/Resolve

Yuki Omiya, Nobuhiro Okabe, Kazuhiro Nakazawa +4

We present high-resolution X-ray spectroscopy of the merging cluster Abell~754 using \textit{XRISM}/Resolve. In GO1 phase, \textit{XRISM}/Resolve observed Abell 754 in two deep poi…

astro-ph.CO2025

XRISM constraints on the velocity power spectrum in the Coma cluster

D. Eckert, M. Markevitch, J. A. ZuHone +6

The velocity field of intracluster gas in galaxy clusters contains key information on the virialization of infalling material, the dissipation of AGN energy into the surrounding me…

astro-ph.GA2025

Comparing XRISM cluster velocity dispersions with predictions from cosmological simulations: are feedback models too ejective?

XRISM Collaboration, Marc Audard, Hisamitsu Awaki +147

The dynamics of the intra-cluster medium (ICM), the hot plasma that fills galaxy clusters, are shaped by gravity-driven cluster mergers and feedback from supermassive black holes (…

astro-ph.GA2025

Suzaku observations of outskirts of nearby clusters and groups: I. electron density and gas fraction to the virial radius

Kyoko Matsushita, Marie Kondo, Kosuke Sato +3

We present an analysis of Suzaku observations of 14 nearby galaxy clusters and groups (z < 0.06), extending radial coverage out to the virial radius (approximately r200). The sampl…