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Globular cluster systems in nearby dwarf galaxies II Nuclear star clusters and their relation to massive Galactic globular clusters

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Academic year: 2020

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Figure

Figure 1. Radial distribution as a function of the absolute magnitude/luminosity for GC candidates in low-mass dwarf galaxies
Figure 2. Left-hand panel: Grey scale F606W band HST/ACS image of UGCA 86. White circles mark all GC candidates selected in Georgiev et al
Figure 3. CMD for nGCs in low-mass dwarf galaxies (squares in panels a and b) and Galactic GCs with extended horizontal branches (EHB-GCs;
Figure 4. Absolute magnitude versus cluster half-light radius r h for nGC in dwarf galaxies (squares in panels a and b) and Galactic GCs with extended horizontal branches (EHB-GCs; large circles in panel b)
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