Статья

CHEERS: The chemical evolution RGS sample

J. de PlaaSRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The NetherlandsJ. S. KaastraLeiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The NetherlandsNorbert WernerDepartment of Theoretical Physics and Astrophysics, Faculty of Science, Masaryk University, Kotlarská 2, 611 37 Brno, Czech RepublicC. PintoInstitute of Astronomy, Madingley Road, Cambridge CB3 0HA, UKPeter KosecInstitute of Astronomy, Madingley Road, Cambridge CB3 0HA, UKYiwei ZhangArgelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, GermanyFrançois MernierLeiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The NetherlandsL. LovisariArgelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, GermanyHiroki AkamatsuSRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The NetherlandsGerrit SchellenbergerArgelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, GermanyF. HofmannMax-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, GermanyT. H. ReiprichArgelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, GermanyA. FinoguenovDepartment of Physics, University of Helsinki, 00014 Helsinki, FinlandJussi AhorantaDepartment of Physics, University of Helsinki, 00014 Helsinki, FinlandJ. S. SandersMax-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, GermanyA. C. FabianInstitute of Astronomy, Madingley Road, Cambridge CB3 0HA, UKO. R. PolsDept. of Astrophysics/IMAPP, Radboud University, PO Box 9010, 6500 GL Nijmegen, The NetherlandsA. SimionescuInstitute of Space and Astronautical Science (ISAS), JAXA, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, 252-5210 Kanagawa, JapanJacco VinkAnton Pannekoek Institute/GRAPPA, University of Amsterdam, PO Box 94249, 1090 GE Amsterdam, The NetherlandsH. BöhringerMax-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany

2017en

ABI

Аннотация

Context. The chemical yields of supernovae and the metal enrichment of the intra-cluster medium (ICM) are not well understood. The hot gas in clusters of galaxies has been enriched with metals originating from billions of supernovae and provides a fair sample of large-scale metal enrichment in the Universe. High-resolution X-ray spectra of clusters of galaxies provide a unique way of measuring abundances in the hot intracluster medium (ICM). The abundance measurements can provide constraints on the supernova explosion mechanism and the initial-mass function of the stellar population. This paper introduces the CHEmical Enrichment RGS Sample (CHEERS), which is a sample of 44 bright local giant ellipticals, groups, and clusters of galaxies observed with XMM-Newton.

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Идентификаторы

DOI: 10.1051/0004-6361/201629926

Цитирования и источники

Цитирований: 2Использованных источников: 0

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