Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 1.

Top panel: orbital decay of GC 5 in runs with low, intermediate, and high resolution. In all cases the GCs reach the center almost at the same time, irrespective of the mass resolution used in GC 5 model. Bottom panel: mass loss of GC 5 in our test runs. Solid lines indicate mass within tidal radius and dashed lines indicate mass within 5 Re.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse