The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars

We use the Illustris simulation to study the relative contributions of in situ star formation and stellar accretion to the build-up of galaxies over an unprecedentedly wide range of masses (M* = 109-1012 M⊙), galaxy types, environments, and assembly histories. We find that the ‘two-phase’ picture of...

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Bibliographic Details
Main Authors: Rodriguez-Gomez, Vicente, Pillepich, Annalisa, Sales, Laura V., Genel, Shy, Zhu, Qirong, Wellons, Sarah, Nelson, Dylan, Springel, Volker, Ma, Chung-Pei, Hernquist, Lars, Vogelsberger, Mark, Torrey, Paul A.
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: Oxford University Press 2017
Online Access:http://hdl.handle.net/1721.1/108509
https://orcid.org/0000-0001-8593-7692
https://orcid.org/0000-0002-5653-0786