The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations

The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations

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© 2021 Oxford University Press. All rights reserved. We study the stellar-to-halo mass relation (SHMR) for central and satellite galaxies with total dynamical masses above 1010.5 M⊙ using the suite of cosmological magnetohydrodynamical simulations IllustrisTNG. In particular, we quantify environment...

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Bibliographic Details
Main Authors: Engler, Christoph (Author), Pillepich, Annalisa (Author), Joshi, Gandhali D (Author), Nelson, Dylan (Author), Pasquali, Anna (Author), Grebel, Eva K (Author), Lisker, Thorsten (Author), Zinger, Elad (Author), Donnari, Martina (Author), Marinacci, Federico (Author), Vogelsberger, Mark (Author), Hernquist, Lars (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor), Massachusetts Institute of Technology. Department of Physics (Contributor)
Format: Article
Language:English
Published: Oxford University Press (OUP), 2022-07-07T18:03:56Z.
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