The origin of the ‘blue tilt’ of globular cluster populations in the E-MOSAICS simulations

ABSTRACT. The metal-poor subpopulation of globular cluster (GC) systems exhibits a correlation between the GC average colour and luminosity, especially in thos

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Bibliographische Detailangaben
Hauptverfasser: Usher, Christopher (VerfasserIn) , Kruijssen, Diederik (VerfasserIn) , Reina-Campos, Marta (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 2018 July 19
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 480, Heft: 3, Pages: 3279-3301
ISSN:1365-2966
DOI:10.1093/mnras/sty1895
Online-Zugang:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty1895
Verlag, Volltext: https://academic.oup.com/mnras/article/480/3/3279/5056200
Volltext
Verfasserangaben:Christopher Usher, Joel Pfeffer, Nate Bastian, J. M. Diederik Kruijssen, Robert A. Crain and Marta Reina-Campos
Beschreibung
Zusammenfassung:ABSTRACT. The metal-poor subpopulation of globular cluster (GC) systems exhibits a correlation between the GC average colour and luminosity, especially in thos
Beschreibung:Gesehen am 20.02.2019
Beschreibung:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty1895