Fig. 6.
Left: remaining mass discrepancy after introducing an exponentially decaying CBM profile with radiative temperature gradient (the IM-CBM solution, cf. Sect. 4.3 and respective column in Table 3), defined as percentage of the dynamical mass of the star. Right: percentage difference between the mass discrepancy after (the IM-CBM solution) and before (the IM solution) the inclusion of CBM in the models.
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