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Fig. 11


The two ionisation states for Titanium, Ti i and Ti ii are compared to our HR sample of Fornax field stars. On the left panel, there is a clear offset of [Ti i/Fe i] versus [Ti ii/Fe i], while on the right panel, [Ti i/Fe i] and [Ti ii/Fe ii] are on a more common scale, showing that ionisation balance is probably not very well achieved in these stars.

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