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Fig. 1
Top: fits of the observed in spectrum G 224-58 A Mg I line triplet, and MgH lines. Labels atoms and atoms+MgH mark synthetic spectra computed with account of atomic lines and atomic lines + MgH, respectively. Middle: dependence of Fa on Vm for Fe lines, model atmosphere 4625/4.5. Bottom: fits to Na I resonance doublet.
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