X-ray observations of the hot gas filling the intra-cluster medium (ICM) provide a wealth of information on the dynamics of clusters of galaxies. The global equilibrium of the ICM is believed to be ensured by non-thermal and thermal pressure support sources, among which gas movements and the dissipation of energy through turbulent motions. Accurate mapping of turbulence using X-ray emission lines is challenging due to the lack of spatially resolved spectroscopy. Only future instruments such as the X-ray Integral Field Unit (X-IFU) on Athena will have the spatial and spectral resolution to quantitatively investigate the ICM turbulence over a broad range of spatial scales. Powerful diagnostics for these studies are line shift and the line bro...
International audienceThe intracluster medium (ICM) in the centers of galaxy clusters is heavily inf...
Astro-H will be able for the first time to map gas velocities and detect turbulence in galaxy cluste...
The general context in which this work fits is introduced in chapter 1. The thesis work presented in...
International audienceX-ray observations of the hot gas filling the intra-cluster medium (ICM) provi...
International audienceX-ray observations of the hot gas filling the intra-cluster medium provide a w...
International audienceX-ray observations of galaxy clusters provide insights on the nature of gaseou...
Context. The X-ray Integral Field Unit (X-IFU) that will be on board the Athena telescope will provi...
International audienceContext. The X-ray Integral Field Unit (X-IFU) that will be on board the Athen...
The hot gas in the intracluster medium (ICM) is perturbed by smooth mass accretion, mergers, feedbac...
International audienceTurbulent processes at work in the intracluster medium perturb this environmen...
The detailed velocity structure of the diffuse X-ray emitting intra-cluster medium (ICM) remains one...
Clusters of galaxies accrete gas, galaxies, and substructures from their larger surroundings. This a...
International audienceThe intracluster medium (ICM) in the centers of galaxy clusters is heavily inf...
Context. Feedback from active galactic nuclei, galactic mergers, and sloshing are thought to give ri...
International audienceThe intracluster medium (ICM) in the centers of galaxy clusters is heavily inf...
Astro-H will be able for the first time to map gas velocities and detect turbulence in galaxy cluste...
The general context in which this work fits is introduced in chapter 1. The thesis work presented in...
International audienceX-ray observations of the hot gas filling the intra-cluster medium (ICM) provi...
International audienceX-ray observations of the hot gas filling the intra-cluster medium provide a w...
International audienceX-ray observations of galaxy clusters provide insights on the nature of gaseou...
Context. The X-ray Integral Field Unit (X-IFU) that will be on board the Athena telescope will provi...
International audienceContext. The X-ray Integral Field Unit (X-IFU) that will be on board the Athen...
The hot gas in the intracluster medium (ICM) is perturbed by smooth mass accretion, mergers, feedbac...
International audienceTurbulent processes at work in the intracluster medium perturb this environmen...
The detailed velocity structure of the diffuse X-ray emitting intra-cluster medium (ICM) remains one...
Clusters of galaxies accrete gas, galaxies, and substructures from their larger surroundings. This a...
International audienceThe intracluster medium (ICM) in the centers of galaxy clusters is heavily inf...
Context. Feedback from active galactic nuclei, galactic mergers, and sloshing are thought to give ri...
International audienceThe intracluster medium (ICM) in the centers of galaxy clusters is heavily inf...
Astro-H will be able for the first time to map gas velocities and detect turbulence in galaxy cluste...
The general context in which this work fits is introduced in chapter 1. The thesis work presented in...