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Fig. 6.

Fig. 6. Refer to the following caption and surrounding text.

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Same KDEs as presented in Fig. 5, but using theoretical masses derived from our MCMC interpolation procedure in the HRD described in Sect. 7.1. Additionally, the right panel shows the estimated mass distributions of the He-rich stars derived by projecting each object to its nearest point along the He-MS (Paczyński 1971) in the HRD.

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