The merger rate of galaxies in the Illustris simulation: a comparison with observations and semi-empirical models

The merger rate of galaxies in the Illustris simulation: a comparison with observations and semi-empirical models

We have constructed merger trees for galaxies in the Illustris simulation by directly tracking the baryonic content of subhaloes. These merger trees are used to calculate the galaxy–galaxy merger rate as a function of descendant stellar mass, progenitor stellar mass ratio, and redshift. We demonstra...

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Bibliographic Details
Main Authors: Rodriguez-Gomez, Vicente, Genel, Shy, Vogelsberger, Mark, Sijacki, Debora, Pillepich, Annalisa, Sales, Laura V., Torrey, Paul, Snyder, Greg, Nelson, Dylan, Springel, Volker, Ma, Chung-Pei, Hernquist, Lars
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: Oxford University Press 2015
Online Access:http://hdl.handle.net/1721.1/98454
https://orcid.org/0000-0001-8593-7692

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http://hdl.handle.net/1721.1/98454
https://orcid.org/0000-0001-8593-7692

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