Lessons learned from 19 years of high-resolution X-ray spectroscopy of galaxy clusters with RGS

TL;DR

This paper reviews 19 years of high-resolution X-ray spectroscopy of galaxy clusters using RGS, highlighting key discoveries about ICM properties, chemical enrichment, and thermal equilibrium.

Contribution

It summarizes the transformative scientific insights gained from RGS data, including the absence of strong cooling flows and detailed chemical and thermal properties of the ICM.

Findings

Lack of strong cooling flows in galaxy clusters

Constraints on ICM turbulence and heating-cooling balance

Detailed chemical enrichment patterns in the ICM

Abstract

The intracluster medium (ICM) contains the vast majority of the baryonic matter in galaxy clusters and is heated to X-ray radiating temperatures. X-ray spectroscopy is therefore a key to understand both the morphology and the dynamics of galaxy clusters. Here we recall crucial evolutionary problems of galaxy clusters unveiled by 19 years of high-resolution X-ray spectroscopy with the Reflection Grating Spectrometer (RGS) on board XMM-Newton. Its exquisite combination of effective area, spectral resolution and excellent performance over two decades enabled transformational science and important discoveries such as the lack of strong cooling flows, the constraints on ICM turbulence and cooling-heating balance. The ability of RGS to resolve individual ICM spectral lines reveals in great detail the chemical enrichment in clusters by supernovae and AGB stars. RGS spectra clearly showed that the ICM plasma is overall in thermal equilibrium which is unexpected given the wealth of energetic phenomena such as jets from supermassive black holes and mergers.