Fossil stellar streams and their globular cluster populations in the E-MOSAICS simulations

ABSTRACT. Stellar haloes encode a fossil record of a galaxy’s accretion history, generally in the form of structures of low surface brightness, such as stellar

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Bibliographische Detailangaben
Hauptverfasser: Hughes, Meghan E. (VerfasserIn) , Kruijssen, Diederik (VerfasserIn) , Reina-Campos, Marta (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 2019
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 482, Heft: 2, Pages: 2795-2806
ISSN:1365-2966
DOI:10.1093/mnras/sty2889
Online-Zugang:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2889
Verlag, Volltext: https://academic.oup.com/mnras/article/482/2/2795/5144774
Volltext
Verfasserangaben:Meghan E. Hughes, Joel Pfeffer, Marie Martig, Nate Bastian, Robert A. Crain, J.M. Diederik Kruijssen and Marta Reina-Campos
Beschreibung
Zusammenfassung:ABSTRACT. Stellar haloes encode a fossil record of a galaxy’s accretion history, generally in the form of structures of low surface brightness, such as stellar
Beschreibung:Gesehen am 18.01.2019
Advance access publication 2018 October 25
Beschreibung:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty2889