XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87
about
Turbulent heating in galaxy clusters brightest in X-rays.CHEERS: The chemical evolution RGS sampleRadial metal abundance profiles in the intra-cluster medium of cool-core galaxy clusters, groups, and ellipticalsStructures and Components in Galaxy Clusters: Observations and ModelsThe origin of the chemical elements in cluster coresEstimating turbulent velocities in the elliptical galaxies NGC 5044 and NGC 5813The metal contents of two groups of galaxiesChemical enrichment in the cluster of galaxies Hydra AMetal-rich multi-phase gas in M 87The gaseous atmosphere of M 87 seen with XMM-NewtonThe uniformity and time-invariance of the intra-cluster metal distribution in galaxy clusters from the IllustrisTNG simulations
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XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87
description
article publié dans la revue scientifique Astronomy and Astrophysics
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im September 2006 veröffentlichter wissenschaftlicher Artikel
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scientific article published in Astronomy and Astrophysics
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wetenschappelijk artikel
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наукова стаття, опублікована у вересні 2006
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name
XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87
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XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87
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type
label
XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87
@en
XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87
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prefLabel
XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87
@en
XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87
@nl
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P2860
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XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87
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J. S. Kaastra
J. de Plaa
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P304
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10.1051/0004-6361:20065678
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2006-09-12T00:00:00Z
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P818
astro-ph/0608177
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2006A&A...459..353W