A census of cool-core galaxy clusters in IllustrisTNG
ABSTRACT. The thermodynamic structure of hot gas in galaxy clusters is sensitive to astrophysical processes and typically difficult to model with galaxy format
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| Hauptverfasser: | , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018 August 03
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 481, Heft: 2, Pages: 1809-1831 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty2078 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2078 Verlag, Volltext: https://academic.oup.com/mnras/article/481/2/1809/5066194 
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| Verfasserangaben: | David J. Barnes, Mark Vogelsberger, Rahul Kannan, Federico Marinacci, Rainer Weinberger, Volker Springel, Paul Torrey, Annalisa Pillepich, Dylan Nelson, Rüdiger Pakmor, Jill Naiman, Lars Hernquist and Michael McDonald |
| Zusammenfassung: | ABSTRACT. The thermodynamic structure of hot gas in galaxy clusters is sensitive to astrophysical processes and typically difficult to model with galaxy format |
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| Beschreibung: | Gesehen am 25.01.2019 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty2078 |