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We present a nucleosynthesis study of the merger of a 0.4 solar masses heliumwhite dwarf with a 0.8 solar masses carbon-oxygen white dwarf, coupling thethermodynamic history of Smoothed Particle Hydrodynamics particles with apost-processing code. The resulting chemical abundance pattern, particularlyfor oxygen and fluorine, is in qualitative agreement with the observedabundances in R Coronae Borealis stars.

White dwarf mergers and the origin of R Coronae Borealis stars