Free Access

Fig. 10


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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.