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PublicationsOpen AccessCOSMICDAWNDiRAC2: 100 Tflop/s HPC cluster pr...HAL Descartes
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  • publication . Article . Preprint . 2017
    How to quench a galaxy
    Open Access English
    Authors:
    Thomas P. Quinn; Fabio Governato; Amélie Saintonge; Hiranya V. Peiris; Michael Tremmel; Nina Roth; Marta Volonteri; Andrew Pontzen;
    doi: 10.1093/mnras/stw2627
    Publisher: HAL CCSD
    Project: NSF | Collaborative Proposal: D... (1410012), EC | BLACK (614199), RCUK | DiRAC2: 100 Tflop/s HPC c... (ST/K000373/1), NSF | Collaborative Research: A... (1514868), EC | COSMICDAWN (306478)

    We show how the interplay between active galactic nuclei (AGN) and merger history determines whether a galaxy quenches star formation at high redshift. We first simulate, in a full cosmological context, a galaxy of total dynamical mass $10^{12}\,M_{\odot}$ at $z=2$. The...

1 research outcomes, page 1 of 1