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- W3103836625 abstract "Many hydrogen-deficient stars are characterized by surface abundance patterns that are hard to reconcile with conventional stellar evolution. Instead, it has been suggested that they may represent the result of a merger episode between a helium and a carbon–oxygen white dwarf. In this Letter, we present a nucleosynthesis study of the merger of a 0.4 M☉ helium white dwarf with a 0.8 M☉ carbon–oxygen white dwarf, by coupling the thermodynamic history of Smoothed Particle Hydrodynamics particles with a post-processing code. The resulting chemical abundance pattern, particularly for oxygen and fluorine, is in qualitative agreement with the observed abundances in R Coronae Borealis stars." @default.
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- W3103836625 date "2011-08-02" @default.
- W3103836625 modified "2023-10-18" @default.
- W3103836625 title "NUCLEOSYNTHESIS DURING THE MERGER OF WHITE DWARFS AND THE ORIGIN OF R CORONAE BOREALIS STARS" @default.
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- W3103836625 doi "https://doi.org/10.1088/2041-8205/737/2/l34" @default.
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