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The fraction of dark matter within galaxies from the IllustrisTNG simulations

ABSTRACT. We use the IllustrisTNG (TNG) cosmological simulations to provide theoretical expectations for the dark matter mass fractions (DMFs) and circular vel

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Bibliographic Details
Main Authors: Lovell, Mark R. (Author) , Pillepich, Annalisa (Author) , Springel, Volker (Author) , Pakmor, Rüdiger (Author) , Weinberger, Rainer (Author)
Format: Article (Journal)
Language:English
Published: 2018 August 17
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 481, Issue: 2, Pages: 1950-1975
ISSN:1365-2966
DOI:10.1093/mnras/sty2339
Online Access:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2339
Verlag, Volltext: https://academic.oup.com/mnras/article/481/2/1950/5079651
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Author Notes:Mark R. Lovell, Annalisa Pillepich, Shy Genel, Dylan Nelson, Volker Springel, Rüdiger Pakmor, Federico Marinacci, Rainer Weinberger, Paul Torrey, Mark Vogelsberger, Adebusola Alabi and Lars Hernquist
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Summary:ABSTRACT. We use the IllustrisTNG (TNG) cosmological simulations to provide theoretical expectations for the dark matter mass fractions (DMFs) and circular vel
Item Description:Gesehen am 24.01.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty2339

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