Figure 17.
The variation of chemical abundances from the LAMOST-SPEMR catalogue with Teff in the three open clusters of Melotte 22, NGC 2682, and NGC 2632. The three colours in the figure correspond to the three open clusters, and the mean μ and standard deviation σ of the chemical abundances are added to each panel.

The variation of chemical abundances from the LAMOST-SPEMR catalogue with Teff in the three open clusters of Melotte 22, NGC 2682, and NGC 2632. The three colours in the figure correspond to the three open clusters, and the mean μ and standard deviation σ of the chemical abundances are added to each panel.

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