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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| Hauptverfasser: | , , , , , , , , , , , , , , , , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
May 9, 2020
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2020, Jahrgang: 495, Heft: 2, Pages: 2247-2264 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/staa1261 |
| Online-Zugang: | 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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| Verfasserangaben: | 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 |
MARC
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| 520 | |a 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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