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The Evolution of Galaxies and Clusters at High Spatial Resolution with Advanced X-ray Imaging Satellite (AXIS)

Russell, Helen R.; Lopez, Laura A.; Allen, Steven W.; Chartas, George; Choudhury, Prakriti Pal; Dupke, Renato A.; Fabian, Andrew C.; Flores, Anthony M.; Garofali, Kristen; Hodges-Kluck, Edmund; Koss, Michael J.; Lanz, Lauranne; Lehmer, Bret D.; Li, Jiang-Tao; Maksym, W. Peter; Mantz, Adam B.; McDonald, Michael; Miller, Eric D.; Mushotzky, Richard F.; Qiu, Yu; Reynolds, Christopher S.; Tombesi, Francesco; Tozzi, Paolo; Trindade-Falcão, Anna; Walker, Stephen A.; Wong, Ka-Wah; Yukita, Mihoko; Zhang, Congyao

The Evolution of Galaxies and Clusters at High Spatial Resolution with Advanced X-ray Imaging Satellite (AXIS) Thumbnail


Authors

Laura A. Lopez

Steven W. Allen

George Chartas

Prakriti Pal Choudhury

Renato A. Dupke

Andrew C. Fabian

Anthony M. Flores

Kristen Garofali

Edmund Hodges-Kluck

Michael J. Koss

Lauranne Lanz

Bret D. Lehmer

Jiang-Tao Li

W. Peter Maksym

Adam B. Mantz

Michael McDonald

Eric D. Miller

Richard F. Mushotzky

Yu Qiu

Christopher S. Reynolds

Francesco Tombesi

Paolo Tozzi

Anna Trindade-Falcão

Stephen A. Walker

Ka-Wah Wong

Mihoko Yukita

Congyao Zhang



Abstract

Stellar and black hole feedback heat and disperse surrounding cold gas clouds, launching gas flows off circumnuclear and galactic disks, producing a dynamic interstellar medium. On large scales bordering the cosmic web, feedback drives enriched gas out of galaxies and groups, seeding the intergalactic medium with heavy elements. In this way, feedback shapes galaxy evolution by shutting down star formation and ultimately curtailing the growth of structure after the peak at redshift 2–3. To understand the complex interplay between gravity and feedback, we must resolve both the key physics within galaxies and map the impact of these processes over large scales, out into the cosmic web. The Advanced X-ray Imaging Satellite (AXIS) is a proposed X-ray probe mission for the 2030s with arcsecond spatial resolution, large effective area, and low background. AXIS will untangle the interactions of winds, radiation, jets, and supernovae with the surrounding interstellar medium across the wide range of mass scales and large volumes driving galaxy evolution and trace the establishment of feedback back to the main event at cosmic noon. This white paper is part of a series commissioned for the AXIS Probe mission concept; additional AXIS white papers can be found at the AXIS website.

Citation

Russell, H. R., Lopez, L. A., Allen, S. W., Chartas, G., Choudhury, P. P., Dupke, R. A., Fabian, A. C., Flores, A. M., Garofali, K., Hodges-Kluck, E., Koss, M. J., Lanz, L., Lehmer, B. D., Li, J.-T., Maksym, W. P., Mantz, A. B., McDonald, M., Miller, E. D., Mushotzky, R. F., Qiu, Y., …Zhang, C. (2024). The Evolution of Galaxies and Clusters at High Spatial Resolution with Advanced X-ray Imaging Satellite (AXIS). Universe, 10(7), Article 273. https://doi.org/10.3390/universe10070273

Journal Article Type Article
Acceptance Date Jun 12, 2024
Online Publication Date Jun 25, 2024
Publication Date 2024-07
Deposit Date Jul 3, 2024
Publicly Available Date Jul 5, 2024
Journal Universe
Print ISSN 2218-1997
Publisher MDPI
Peer Reviewed Peer Reviewed
Volume 10
Issue 7
Article Number 273
DOI https://doi.org/10.3390/universe10070273
Keywords X-rays; instrumentation; galaxies; clusters; feedback
Public URL https://nottingham-repository.worktribe.com/output/36868712
Publisher URL https://www.mdpi.com/2218-1997/10/7/273

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