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Fig. A.1


Illustration of the polynomial fit (black dashed line) to the distribution of Hα luminosity and Mst (filled dots) for the model DDC15 at 200 d, together with the correlation obtained by Botyánszki et al. (2018) for their models at 200 d. Their Eq. (1) should read Y = 40.0 + 0.17X − 0.2X2, with the nomenclature given in the caption of our Table A.1 above.

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