Constraining nuclear star cluster formation using MUSE-AO observations of the early-type galaxy FCC 47
Context. Nuclear star clusters (NSCs) are found in at least 70% of all galaxies, but their formation path is still unclear. In the most common scenarios, NSCs form in-situ from the galaxy's central gas reservoir, through the merging of globular clusters (GCs), or through a combination of both. Aims: As the scenarios pose different expectations for
Fahrion, Katja et al.
Fecha de publicación:
8
2019