First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time

First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time

We present a new cosmological, magnetohydrodynamical simulation for galaxy formation: TNG50, the third and final instalment of the IllustrisTNG project. TNG50 evolves 2 × 21603 dark matter particles and gas cells in a volume 50 comoving Mpc across. It hence reaches a numerical resolution typical of...

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Bibliographic Details
Main Authors: Pillepich, Annalisa (Author), Nelson, Dylan (Author), Springel, Volker (Author), Pakmor, Rüdiger (Author), Torrey, Paul (Author), Weinberger, Rainer (Author), Vogelsberger, Mark (Author), Marinacci, Federico (Author), Genel, Shy (Author), van der Wel, Arjen (Author), Hernquist, Lars (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: Oxford University Press (OUP), 2020-11-17T22:01:12Z.
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