The evolution of planetary nebulae - VII. Modelling planetary nebulae of distant stellar systems

Free Access

Fig. 29

Open with DEXTER Download original image

The same data and theoretical sequences as presented in Fig. 28, but now plotted over M(Hα + [N ii]). Objects and sequences are only plotted down to M(5007) = 1, the brightness limit of the samples (cf. Fig. 28).

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.