The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
© 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...
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) |
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Format: | Article |
Language: | English |
Published: |
Oxford University Press (OUP),
2022-05-06T17:05:19Z.
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Subjects: | |
Online Access: | Get fulltext |
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