Fig. 13.
Elemental composition ratios ratio of the bound remnant and the unbound ejecta of the G14 simulation with respect to Fe and relative to the solar ratio. The black points are the spectroscopically determined composition of the atmosphere of the white dwarf LP 40-365 from Raddi et al. (2018). While the Ca, Ti, Cr, Fe and Ni abundances relative to Fe fit very well, the lighter elements are in distinct tension with the measurements.
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