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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 6.

Twin-axis plot of orbital decay and mass loss of GCs in IC 2. Dark- and light-gray lines represent the total mass within tidal radius and 5Re (equivalent to half-mass radius). Vertical dashed lines represent the time each GC merged at the center.

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