Low-metallicity CO + He WD post-merger models for RCB stars as a source of pre-solar graphite grains

1Menon, A.,1Karakas, A.I.,2Lugaro, M.,1,2Doherty, C.L.,3,4,5Ritter, C.
Monthly Notices of the Royal Astronomical Society 482, 2320-2335 Link to Article [DOI: 10.1093/mnras/sty2606]
1Monash Centre for Astrophysics (MoCA), School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia
2Konkoly Observatory, Hungarian Academy of Sciences, Konkoly-Thege Miklos ut 15-17, Budapest, 1121, Hungary
3Astrophysics Group, Keele University, Keele, Staffordshire, ST5 5BG, United Kingdom

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