Halo mass estimates from the globular cluster populations of 175 low surface brightness galaxies in the Fornax cluster

Abstract. The halo masses Mhalo of low surface brightness (LSB) galaxies are critical measurements for understanding their formation processes. One promising m

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Bibliographic Details
Main Authors: Prole, Daniel J. (Author) , Wittmann, Carolin (Author)
Format: Article (Journal)
Language:English
Published: 2019 February 1
In: Monthly notices of the Royal Astronomical Society
Year: 2019, Volume: 484, Issue: 4, Pages: 4865-4880
ISSN:1365-2966
DOI:10.1093/mnras/stz326
Online Access:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/stz326
Verlag, Volltext: https://academic.oup.com/mnras/article/484/4/4865/5305864
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Author Notes:D.J. Prole, M. Hilker, R.F.J. van der Burg, M. Cantiello, A. Venhola, E. Iodice, G. van de Ven, C. Wittmann, R.F. Peletier, S. Mieske, M. Capaccioli, N. R. Napolitano, M. Paolillo, M. Spavone and E. Valentijn
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Summary:Abstract. The halo masses Mhalo of low surface brightness (LSB) galaxies are critical measurements for understanding their formation processes. One promising m
Item Description:Gesehen am 18.02.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stz326