The diverse evolutionary paths of simulated high-

The diverse evolutionary paths of simulated high-

Massive quiescent galaxies have much smaller physical sizes at high redshift than today. The strong evolution of galaxy size may be caused by progenitor bias, major and minor mergers, adiabatic expansion, and/or renewed star formation, but it is difficult to test these theories observationally. Here...

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Bibliographic Details
Main Authors: Wellons, Sarah, Ma, Chung-Pei, Rodriguez-Gomez, Vicente, Pillepich, Annalisa, Nelson, Dylan, Genel, Shy, Hernquist, Lars, Torrey, Paul A., Vogelsberger, Mark
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:en_US
Published: Oxford University Press 2017
Online Access:http://hdl.handle.net/1721.1/108527
https://orcid.org/0000-0002-5653-0786
https://orcid.org/0000-0001-8593-7692

Internet

http://hdl.handle.net/1721.1/108527
https://orcid.org/0000-0002-5653-0786
https://orcid.org/0000-0001-8593-7692

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