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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 5.

Surface-density profile of UGC 7346 + NSC1, NSC2, and NSC3 (from top to bottom, respectively). Dashed–dotted line shows the surface brightness profile of UGC 7346 at t = 0. Middle panel: surface density of NSC1 is shown as a solid gray line for comparison. Bottom panel: solid gray line represents the surface density of NSC3 at 1.6 Gyr. Thin dashed lines show the surface density of the clusters C1 and C2 observed in IC 3.

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