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Giant clumps in simulated high-z galaxies: properties, evolution and dependence on feedback

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We study the evolution and properties of giant clumps in high-z disc galaxies using adaptive mesh refinement cosmological simulations at redshifts z ∼ 6-1. Our sample consists of 34 galaxies, of halo masses 1011-1012 M⊙ at z = 2, run with and without radiation pressure (RP) feedback from young stars...

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Main Authors: Mandelker, Nir (Author) , Ceverino, Daniel (Author)
Format: Article (Journal)
Language:English
Published: 16 September 2016
In: Monthly notices of the Royal Astronomical Society
Year: 2017, Volume: 464, Issue: 1, Pages: 635-665
ISSN:1365-2966
DOI:10.1093/mnras/stw2358
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stw2358
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Author Notes:Nir Mandelker, Avishai Dekel, Daniel Ceverino, Colin DeGraf, Yicheng Guo and Joel Primack
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Giant clumps in simulated high-z galaxies: properties, evolution and dependence on feedback by Mandelker, Nir (Author) , Ceverino, Daniel (Author) ,


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