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NEW HUBBLE SPACE TELESCOPE WFC3/UVIS OBSERVATIONS AUGMENT THE STELLAR POPULATION COMPLEXITY OF omega CENTAURI

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Figure

Figure 1. Collection of CMDs from our three data sets: the WFC3/UVIS CMD in the UV filters m F275W vs
Figure 2. Definition of the main CMD branches used in this paper.
Figure 4. Example of the definition of the MS RLs.
Figure 5. bMS and the MS-a run almost parallel in all CMDs. In some CMDs, the MS-a seems to cross the rMS.
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