Resolving small-scale cold circumgalactic gas in TNG50
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. We use the high-resolution TNG50 cosmological magnetohydrodynamical simulation to explore the properties and origin of cold circumgalactic medium (CGM) gas around massive galaxies (M 1011 M) at int...
Main Authors: | Nelson, Dylan, Sharma, Prateek, Pillepich, Annalisa, Springel, Volker, Pakmor, Rüdiger, Weinberger, Rainer, Vogelsberger, Mark, Marinacci, Federico, Hernquist, Lars |
---|---|
Other Authors: | MIT Kavli Institute for Astrophysics and Space Research |
Format: | Article |
Language: | English |
Published: |
Oxford University Press (OUP)
2022
|
Online Access: | https://hdl.handle.net/1721.1/142404 |
Similar Items
-
First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback
by: Nelson, Dylan, et al.
Published: (2021) -
First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback
by: Nelson, Dylan, et al.
Published: (2022) -
Ejective and preventative: the IllustrisTNG black hole feedback and its effects on the thermodynamics of the gas within and around galaxies
by: Zinger, Elad, et al.
Published: (2021) -
First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time
by: Pillepich, Annalisa, et al.
Published: (2020) -
Simulating Galaxy Formation with the IllustrisTNG Model
by: Pillepich, Annalisa, et al.
Published: (2021)