First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
The IllustrisTNG project is a new suite of cosmological magnetohydrodynamical simulations of galaxy formation performed with the arepo code and updated models for feedback physics. Here, we introduce the first two simulations of the series, TNG100 and TNG300, and quantify the stellar mass content of...
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| Hauptverfasser: | , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 475, Heft: 1, Pages: 648-675 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stx3112 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx3112 Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/475/1/648/4683271 
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| Verfasserangaben: | Annalisa Pillepich, Dylan Nelson, Lars Hernquist, Volker Springel, Rüdiger Pakmor, Paul Torrey, Rainer Weinberger, Shy Genel, Jill P. Naiman, Federico Marinacci, Mark Vogelsberger |
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First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
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