Orateur
Stefano Ettori
(INAF-Osservatorio di Astrofisica e Scienza dello Spazio in Bologna)
Description
I will discuss how current (with XMM-Newton) and future X-ray observations (with XRISM and Athena) will be able to characterize the non-thermal pressure support in galaxy clusters, and how we can convert it in an estimate of the hydrostatic mass bias, also for a cosmological purpose.
Auteur principal
Stefano Ettori
(INAF-Osservatorio di Astrofisica e Scienza dello Spazio in Bologna)
