Fig. 7
Luminosity function of LMC J-stars (JSLF). Number fraction (NJ/NC) of J-stars among C-stars for post-nova mergers and HBB-stars excluding Case-B RLOF binary mergers is shown with observed J-stars from the sample of Morgan et al. (2003) binned in MBol intervals of 0.5 mag. The total NJ/NC ratio is ~2% for the nova-polluted mergers – lower than the total NJ/NC in Fig. 6 (~5%) and the observed fraction (~10%) of the stars in the sample of Morgan et al. (2003).
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