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The Next Generation Fornax Survey (NGFS): VII. A MUSE view of the nuclear star clusters in Fornax dwarf galaxies

ABSTRACT. Clues to the formation and evolution of nuclear star clusters (NSCs) lie in their stellar populations. However, these structures are often very faint

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Main Authors: Johnston, Evelyn J. (Author) , Puzia, Thomas H. (Author) , D’Ago, Giuseppe (Author) , Eigenthaler, Paul (Author) , Galaz, Gaspar (Author) , Häußler, Boris (Author) , Mora, Marcelo D. (Author) , Ordenes Briceño, Yasna (Author) , Rong, Yu (Author) , Spengler, Chelsea (Author) , Vogt, Frédéric (Author) , Côté, Patrick (Author) , Grebel, Eva K. (Author) , Hilker, Michael (Author) , Mieske, Steffen (Author) , Miller, Bryan (Author) , Sánchez-Janssen, Ruben (Author) , Taylor, Matthew A. (Author) , Zhang, Hong-Xin (Author)
Format: Article (Journal)
Language:English
Published: May 9, 2020
In: Monthly notices of the Royal Astronomical Society
Year: 2020, Volume: 495, Issue: 2, Pages: 2247-2264
ISSN:1365-2966
DOI:10.1093/mnras/staa1261
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/staa1261
Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/495/2/2247/5835231
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Author Notes:Evelyn J. Johnston, Thomas H. Puzia, Giuseppe D’Ago, Paul Eigenthaler, Gaspar Galaz, Boris Häußler, Marcelo D. Mora, Yasna Ordenes-Briceño, Yu Rong, Chelsea Spengler, Frédéric Vogt, Patrick Côté, Eva K. Grebel, Michael Hilker, Steffen Mieske, Bryan Miller, Ruben Sánchez-Janssen, Matthew A. Taylor and Hong-Xin Zhang
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Summary:ABSTRACT. Clues to the formation and evolution of nuclear star clusters (NSCs) lie in their stellar populations. However, these structures are often very faint
Item Description:Gesehen am 18.08.2020
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/staa1261

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