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GLOBULAR CLUSTER SYSTEMS IN BRIGHTEST CLUSTER GALAXIES. III. BEYOND BIMODALITY

  • Authors: William E. Harris, Stephanie M. Ciccone, Gwendolyn M. Eadie, Oleg Y. Gnedin, Douglas Geisler, Barry Rothberg, and Jeremy Bailin

2017 The Astrophysical Journal 835 101.

  • Provider: AAS Journals

Caption: Figure 6.

Locations of the measured starlike objects brighter than ﹩F814W=27.0﹩ in the ACS field centered near UGC 9799 (left panel) and in the Parallel WFC3 field (right panel). Fiducial directions on the sky (north, east) are marked in both panels. Small red circles mark smaller companion galaxies with GC populations of their own, as listed in the text. For WFC3, the red dashed line indicates the border between contaminating small galaxies (above the line) and a cleaner sample of IGC GCs (below the line).

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