XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87 - Wikidata - awgldk - TriplyDB

XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87

XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87

http://www.wikidata.org/entity/Q55893402

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Turbulent heating in galaxy clusters brightest in X-rays.CHEERS: The chemical evolution RGS sample Radial metal abundance profiles in the intra-cluster medium of cool-core galaxy clusters, groups, and ellipticals Structures and Components in Galaxy Clusters: Observations and Models The origin of the chemical elements in cluster cores Estimating turbulent velocities in the elliptical galaxies NGC 5044 and NGC 5813 The metal contents of two groups of galaxies Chemical enrichment in the cluster of galaxies Hydra A Metal-rich multi-phase gas in M 87 The gaseous atmosphere of M 87 seen with XMM-Newton The 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

http://www.wikidata.org/entity/Q55893402

description

article publié dans la revue scientifique Astronomy and Astrophysics

@fr

im September 2006 veröffentlichter wissenschaftlicher Artikel

@de

scientific article published in Astronomy and Astrophysics

@en

wetenschappelijk artikel

@nl

наукова стаття, опублікована у вересні 2006

@uk

name

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

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

@nl

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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0004-6361:20065678

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Astronomy and Astrophysics

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XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87

@en

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J. S. Kaastra

http://www.w3.org/2001/XMLSchema#string

J. Vink

http://www.w3.org/2001/XMLSchema#string

J. de Plaa

http://www.w3.org/2001/XMLSchema#string

N. Werner

http://www.w3.org/2001/XMLSchema#string

P2860

Chemical composition of 90 F and G disk dwarfs

The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances

Solar System Abundances and Condensation Temperatures of the Elements

X-ray evidence for spectroscopic diversity of type Ia supernovae: XMM observation of the elemental abundance pattern in M87

M87 at 90 Centimeters: A Different Picture

The Reflection Grating Spectrometer on board XMM-Newton

Chemical evolution in Sérsic 159-03 observed with XMM-Newton

XMM-Newton spectroscopy of the cluster of galaxies 2A 0335+096

The temperature structure in the core of Sérsic 159-03

On the Temperature Structure of M87

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353–360

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scholarly article

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10.1051/0004-6361:20065678

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2

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459

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Aurora Simionescu

Hans Böhringer

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2006-09-12T00:00:00Z

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43104285

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astro-ph/0608177

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2006A&A...459..353W

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