Large-scale mass distribution in the Illustris simulation
Observations at low redshifts thus far fail to account for all of the baryons expected in the Universe according to cosmological constraints. A large fraction of the baryons presumably resides in a thin and warm–hot medium between the galaxies, where they are difficult to observe due to their low de...
Main Authors: | Haider, M., Steinhauser, D., Genel, S., Springel, V., Hernquist, L., Vogelsberger, Mark, Torrey, Paul A. |
---|---|
Other Authors: | Massachusetts Institute of Technology. Department of Physics |
Format: | Article |
Language: | en_US |
Published: |
Oxford University Press
2017
|
Online Access: | http://hdl.handle.net/1721.1/108540 https://orcid.org/0000-0001-8593-7692 https://orcid.org/0000-0002-5653-0786 |
Similar Items
-
The star formation main sequence and stellar mass assembly of galaxies in the Illustris simulation
by: Sparre, Martin, et al.
Published: (2015) -
Hydrogen reionization in the Illustris universe
by: Bauer, Andreas, et al.
Published: (2017) -
The large-scale distribution of ionized metals in IllustrisTNG
by: Artale, M Celeste, et al.
Published: (2022) -
The Illustris simulation: the evolving population of black holes across cosmic time
by: Sijacki, Debora, et al.
Published: (2017) -
Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the Universe
by: Vogelsberger, Mark, et al.
Published: (2015)