Mapping the Perseus galaxy cluster with XRISM: Gas kinematic features and their implications for turbulence
Congyao Zhang(University of Chicago), Norbert Werner, John ZuHone, Koji Mori(University of Miyazaki), Nhut Truong(Goddard Space Flight Center), Anna Ogorzalek(Goddard Space Flight Center), Yutaka Fujita, Eugene Churazov, Eric Haynes Miller, Yuto Ichinohe, Hiroshi Nakajima, Maxim Markevitch, Julie Hlavacek-Larrondo, Megan E. Eckart, Frederick S. Porter, Irina Zhuravleva, Ay?egü Tümer, François Mernier, Elena Bellomi(Center for Astrophysics Harvard & Smithsonian), Kyoko Matsushita, Shutaro Ueda(Kanazawa University)
Cited by 0
Related Papers
3D chemical structure of diffuse turbulent ISM
|Astronomy and Astrophysics|2020|41
Statistical description of dust polarized emission from the diffuse interstellar medium
|Springer Link (Chiba Institute of Technology)|2020|35
Spectral index of synchrotron emission: insights from the diffuse and magnetised interstellar medium
|Astronomy and Astrophysics|2021|24
3D chemical structure of the diffuse turbulent interstellar medium
|Astronomy and Astrophysics|2022|16
ICM-SHOX. I. Methodology Overview and Discovery of a Gas–Dark Matter Velocity Decoupling in the MACS J0018.5+1626 Merger
|The Astrophysical Journal|2024|11