Anomalously low-mass core-He-burning star in NGC 6819 as a post-common-envelope phase product

Open Access

Fig. 8.

Same as Figure 4, but for the subsample described in Sect. 4.2 (see also Table 3). Effective temperatures above 8000 K are not included in the figure for clarity. As explained in Appendix A, we take the age that gives the highest likelihood as the reference time for the CHeB of each MC simulation.

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