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...
Main Authors: | Schaal, Kevin (Author), Springel, Volker (Author), Pakmor, Rüdiger (Author), Pfrommer, Christoph (Author), Nelson, Dylan (Author), Vogelsberger, Mark (Contributor), Genel, Shy (Author), Pillepich, Annalisa (Author), Sijacki, Debora (Author), Hernquist, Lars (Author) |
---|---|
Other Authors: | Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor) |
Format: | Article |
Language: | English |
Published: |
Oxford University Press,
2017-05-01T18:20:03Z.
|
Subjects: | |
Online Access: | Get fulltext |
Similar Items
-
Hydrogen reionization in the Illustris universe
by: Bauer, Andreas, et al.
Published: (2017) -
Reducing noise in moving-grid codes with strongly-centroidal Lloyd mesh regularization
by: Mocz, Philip, et al.
Published: (2017) -
The colours of satellite galaxies in the Illustris simulation
by: Sales, Laura V., et al.
Published: (2015) -
The fraction of dark matter within galaxies from the IllustrisTNG simulations
by: Lovell, Mark R., et al.
Published: (2019) -
Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the Universe
by: Vogelsberger, Mark, et al.
Published: (2015)