Reproducing the observed abundances in RCB and HdC stars with post-double-degenerate merger models - constraints on merger and post-merger simulations and physics processes

Physics & Astronomy

• augmentation 23%
• coronas 77%
• envelopes 50%
• hydrodynamics 14%
• hydrogen 12%
• nuclear fusion 61%
• oxygen 11%
• physics 49%
• R Coronae Borealis stars 100%
• simulation 29%
• stars 53%
• stellar evolution 23%
• temperature 5%
• variable stars 24%

Earth & Environmental Sciences

• corona 86%
• hydrodynamics 4%
• hydrogen 5%
• isotopic ratio 21%
• merger 98%
• oxygen 4%
• physical process 5%
• physics 64%
• shell 10%
• simulation 34%
• temperature 2%