Shock finding on a moving-mesh: II. Hydrodynamic shocks in the Illustris universe
Hydrodynamical shocks are a manifestation of the non-linearity of the Euler equations and play a fundamental role in cosmological gas dynamics. In this work, we identify and analyse shocks in the Illustris simulation, and contrast the results with those of non-radiative runs. We show that simulation...
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| Main Authors: | , , , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
04 July 2016
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2016, Volume: 461, Issue: 4, Pages: 4441-4465 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stw1587 |
| Online Access: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stw1587 |
| Author Notes: | Kevin Schaal, Volker Springel, Rüdiger Pakmor, Christoph Pfrommer, Dylan Nelson, Mark Vogelsberger, Shy Genel, Annalisa Pillepich, Debora Sijacki and Lars Hernquist |
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Shock finding on a moving-mesh: II. Hydrodynamic shocks in the Illustris universe
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