Advances in Galaxy Clusters
A special issue of Applied Sciences (ISSN 2076-3417). This special issue belongs to the section "Aerospace Science and Engineering".
Deadline for manuscript submissions: closed (28 February 2023) | Viewed by 2416
Special Issue Editor
Special Issue Information
Dear Colleagues,
The science of galaxy clusters is entering a new era. Upcoming X-ray missions promise to provide important clues on galaxy cluster physics, from the chemical evolution of the intracluster medium to the non-thermal motions prevalent therein. The former will shed light on the origin of various elements, be it SNe Ia or SNcc, while the latter will test models of AGN feedback and will assess any biases that may enter the cosmological utility of galaxy clusters. Furthermore, upcoming radio projects will shed light on the high-energy particle content of clusters, as well as on the role of the magnetic fields that permeat their atmospheres.
This Special Issue invites observational and theoretical papers in anticipation and in support of these upcoming developments, including on atomic data that will maximize the spectroscopic value of upcoming X-ray missions.
Dr. Marios Chatzikos
Guest Editor
Manuscript Submission Information
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