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(1 - 6 of 6)
The birth of a relativistic jet following the disruption of a star by a cosmological black hole
Radial metal abundance profiles in the intra-cluster medium of cool-core galaxy clusters, groups, and ellipticals
CHEERS: The chemical evolution RGS sample
Origin of central abundances in the hot intra-cluster medium. I. Individual and average abundance ratios from XMM-Newton EPIC
Origin of central abundances in the hot intra-cluster medium. II. Chemical enrichment and supernova yield models
Chemical enrichment in the hot intra-cluster medium seen with XMM-Newton/EPIC