Free Access
Fig. 3
Observed PN luminosity function for: a) the whole sample, b) the PNe in the central zone, and c) the PNe in the outskirts of NGC 300. Bin sizes are described in the text. The errors bars correspond to the Poissonian error. Solid lines represent our best fit of the empirical PNLF for the four brightest bins in each case.
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.