Constraining r-process nucleosynthesis with multi-objective Galactic chemical evolution models

Open Access

Fig. 2

Predicted model curves of [Eu/Fe] vs [Fe/H] (left column) for fixed combinations of three out of the four input parameters (Y_Eu,r, α, [M_l, M_u], τ) shown alongside the corresponding $χ_{Eu}^{2}$ $Mathematical equation: $\chi _{{\rm{Eu}}}^2$$ values as a function of the fourth parameter (right column). In the left column, curve colours indicate the associated $χ_{Eu}^{2}$ $Mathematical equation: $\chi _{{\rm{Eu}}}^2$$ values.

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