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Formation of a Nuclear Star Cluster through the Inspiral of Globular Clusters: A Case Study of the Dwarf Elliptical Galaxy UGC 7346

  • Authors: Ismael Khan, Fazeel Mahmood Khan, Andrea V. Macciò, Kelly Holley-Bockelmann, Peter Berczik

Ismael Khan et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 9.

Comparison of our obtained NSC masses with NSCs in literature. The samples from R. Sánchez-Janssen et al. (2019) and C. Spengler et al. (2017) represent Virgo Cluster NSCs. The samples from I. Y. Georgiev et al. (2016) and P. Erwin & D. A. Gadotti (2012) represent late-type field spirals, and R. Pechetti et al. (2020) represents local volume galaxies. The dashed black line represents the MgalMnsc scaling relation presented by N. Neumayer et al. (2020), and the solid black line shows the scaling relation for early-type galaxies by I. Y. Georgiev et al. (2016). The red and purple crosses represent NSC1 and NSC2, and the black cross represents the NSC3.

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