Fig. 6.

Central panels: Na ID absorption (Abs.) and emission (Em.) line fluxes across the FOV obtained by integrating for each spaxel the spectra in the regions 5860 − 5910 Å and 5890 − 5920 Å, respectively. Negative and positive fluxes were obtained after subtracting the stellar contribution (pPXF best fit); for the absorption fluxes, we also removed the He I emission line (simultaneous best-fit results). Insets: different spectra extracted from the regions labelled in the flux maps, with normalised fluxes: absorption- (emission-) dominated Na ID line profiles are shown in the right (left) panels. Red curves represent the Na ID stellar contribution fitted with pPXF, rescaled for visual purposes. Vertical dashed lines indicate the (NW nucleus systemic) wavelengths of the He I and Na ID doublet lines.
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.