Modelling R Coronae Borealis stars: effects of He-burning shell temperature and metallicity
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DOI: 10.1093/mnras/staa2526
Abstract: The R Coronae Borealis (RCB) stars are extremely hydrogen-deficient carbon stars which produce large amounts of dust, causing sudden deep declines in brightness. They are believed to be formed primarily through white dwarf mergers. In… read more here.
Keywords: temperature; burning shell; shell temperature; metallicity ... See more keywords