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- W1775796076 abstract "We present a nucleosynthesis study of the merger of a 0.4 solar masses helium white dwarf with a 0.8 solar masses carbon-oxygen white dwarf, 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.
- W1775796076 created "2016-06-24" @default.
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- W1775796076 date "2011-10-09" @default.
- W1775796076 modified "2023-10-18" @default.
- W1775796076 title "White dwarf mergers and the origin of R Coronae Borealis stars" @default.
- W1775796076 doi "https://doi.org/10.48550/arxiv.1110.1855" @default.
- W1775796076 hasPublicationYear "2011" @default.
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