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Properties of HI discs in the Auriga cosmological simulations

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We analyse the properties of the H i gas distribution in the Auriga project, a set of magnetohydrodynamic cosmological simulations performed with the moving-mesh code arepo and a physics model for galaxy formation that succeeds in forming realistic late-type galaxies in the 30 Milky Way-sized haloes...

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Main Authors: Marinacci, Federico (Author) , Grand, Robert J. J. (Author) , Pakmor, Rüdiger (Author) , Springel, Volker (Author) , Gómez, Facundo A. (Author) , Frenk, Carlos (Author) , White, Simon D. M. (Author)
Format: Article (Journal)
Language:English
Published: 2017 January 18
In: Monthly notices of the Royal Astronomical Society
Year: 2017, Volume: 466, Issue: 4, Pages: 3859-3875
ISSN:1365-2966
DOI:10.1093/mnras/stw3366
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stw3366
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Author Notes:Federico Marinacci, Robert J.J. Grand, Rüdiger Pakmor, Volker Springel, Facundo A. Gómez, Carlos S. Frenk and Simon D.M. White
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Properties of HI discs in the Auriga cosmological simulations by Marinacci, Federico (Author) , Grand, Robert J. J. (Author) , Pakmor, Rüdiger (Author) , Springel, Volker (Author) , Gómez, Facundo A. (Author) , Frenk, Carlos (Author) , White, Simon D. M. (Author) ,


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