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No cores in dark matter-dominated dwarf galaxies with bursty star formation histories

ABSTRACT. Measurements of the rotation curves of dwarf galaxies are often interpreted as requiring a constant density core at the centre, at odds with the ‘cus

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Bibliographic Details
Main Authors: Bose, Sownak (Author) , Grand, Robert J. J. (Author) , Pakmor, Rüdiger (Author) , Springel, Volker (Author)
Format: Article (Journal)
Language:English
Published: 2019 April 29
In: Monthly notices of the Royal Astronomical Society
Year: 2019, Volume: 486, Issue: 4, Pages: 4790-4804
ISSN:1365-2966
DOI:10.1093/mnras/stz1168
Online Access:Verlag, Volltext: https://doi.org/10.1093/mnras/stz1168
Verlag, Volltext: https://academic.oup.com/mnras/article/486/4/4790/5481533
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Author Notes:Sownak Bose, Carlos S. Frenk, Adrian Jenkins, Azadeh Fattahi, Facundo A. Gómez, Robert J.J. Grand, Federico Marinacci, Julio F. Navarro, Kyle A. Oman, Rüdiger Pakmor, Joop Schaye, Christine M. Simpson and Volker Springel
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Summary:ABSTRACT. Measurements of the rotation curves of dwarf galaxies are often interpreted as requiring a constant density core at the centre, at odds with the ‘cus
Item Description:Gesehen am 03.06.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stz1168

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