The LEGARE Project - I. Chemical evolution model of the Nuclear Stellar Disc in a Bayesian framework

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Fig. 7

Results of Model ENR. Upper panel: as in Fig. 3, but compared to the MDF obtained by using the Sample B (filled purple distribution; see Section 3 for details) and the predictions of the best-fit Model ENR (with parameters listed in Table 1). Lower panel: as in Fig. 4, but for Model ENR.

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