The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way

ABSTRACT. We present a detailed comparison of the Milky Way (MW) globular cluster (GC) kinematics with the 25 MW-mass cosmological simulations from the E-MOSAIC

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Bibliographic Details
Main Authors:	Trujillo-Gomez, Sebastian (Author) , Kruijssen, Diederik (Author) , Reina-Campos, Marta (Author) , Pfeffer, Joel L. (Author) , Keller, Benjamin W. (Author) , Crain, Robert A. (Author) , Bastian, Nate (Author) , Hughes, Meghan E. (Author)
Format:	Article (Journal)
Language:	English
Published:	2021 February 6
In:	Monthly notices of the Royal Astronomical Society Year: 2021, Volume: 503, Issue: 1, Pages: 31-58
ISSN:	1365-2966
DOI:	10.1093/mnras/stab341
Online Access:	Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stab341 Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/503/1/31/6129790
Author Notes:	Sebastian Trujillo-Gomez, J.M. Diederik Kruijssen, Marta Reina-Campos, Joel L. Pfeffer, Benjamin W. Keller, Robert A. Crain, Nate Bastian and Meghan E. Hughes

Description
Summary:	ABSTRACT. We present a detailed comparison of the Milky Way (MW) globular cluster (GC) kinematics with the 25 MW-mass cosmological simulations from the E-MOSAIC
Item Description:	Gesehen am 21.06.2021
Physical Description:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/stab341