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Fig. 10

image

MUSE spectra of 3 stars in the globular cluster NGC 6 397. The reduced data appear in black, while the spectra corrected by the synthetic spectrum determined by molecfit are shown in red. The molecular column densities and line spread function were determined using only star #5326 (bottom) located on IFU #7: the results were used on the spectra of star #10327, also located on IFU #7 (middle), and #10893 (top), located on IFU #13. The yellow shaded areas indicate the inclusion regions. No regions were excluded from the fit.

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