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We have undertaken a detailed abundance analysis of the optical counterpartof the IR source IRAS16559-2957 with the aim of confirming its possiblepost-AGB nature. The star shows solar metallicity and our investigation of alarge number of elements including CNO and 12C/13C suggests that this objecthas experienced the first dredge-up and it is likely still at RGB stage.

Detailed atmospheric abundance analysis of the optical counterpart of the IR source IRAS 16559-2957