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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Main Authors: Pillepich, Annalisa, Nelson, Dylan, Springel, Volker, Pakmor, Rüdiger, Torrey, Paul, Weinberger, Rainer, Vogelsberger, Mark, Marinacci, Federico, Genel, Shy, van der Wel, Arjen, Hernquist, Lars
其他作者: MIT Kavli Institute for Astrophysics and Space Research
格式: Article
語言:English
出版: Oxford University Press (OUP) 2020
在線閱讀:https://hdl.handle.net/1721.1/128510