Galactic archaeology with [Mg/Mn] versus [Al/Fe] abundance ratios - Uncertainties and caveats

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Table 3.

Yield correction adopted in MIX MW model and MIX LMC model.

Prescriptions of MIX MW and MIX LMC models
Element	LIMS	Massive stars	SNIa
	(Karakas 2010)	(Kobayashi et al. 2006)	(Iwamoto et al. 1999)

Fe	✓	×0.7	✓
Mg	✓	Z ∈ (3 − 8)×10⁻³ → ×1.2	✓
		Z > 8 × 10⁻³ → ×(Z/0.004)^0.4
Al	Z > 8 × 10⁻³ → ×0.8	×1.5	✓
Mn	✓	✓	✓

Notes. In these two models, we adopted the corrections already introduced in Table 2 for Mg, Fe, and Al. Regarding Mn, we adopted the original prescriptions since, as displayed in the right panel of Fig. 2, they are the best at reproducing the observed abundance ratio.

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