The MUSE-Faint survey

Aims. It has been shown that the ultra-faint dwarf galaxy Eridanus 2 may host a stellar cluster in its centre. If this cluster is shown to exist, it can be used to set constraints on the mass and abundance of massive astrophysical compact halo objects (MACHOs) as a form of dark matter. Previous rese...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2020-03, Vol.635
Hauptverfasser:	Zoutendijk, Sebastiaan L, Brinchmann, Jarle, Boogaard, Leindert A, Madusha L. P. Gunawardhana, Tim-Oliver Husser, Kamann, Sebastian, Andrés Felipe Ramos Padilla, Roth, Martin M, Bacon, Roland, den Brok, Mark, Dreizler, Stefan, Krajnović, Davor
Format:	Artikel
Sprache:	eng
Schlagworte:	Carbon stars Confidence intervals Dark matter Dwarf galaxies Line of sight Star clusters Stellar age Very Large Telescope
Online-Zugang:	Volltext
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