Free Access

Fig. 15

image

Classical HRD and surface N abundances as a function of log LL and Teff for the sample stars plotted against the current Geneva (left) and the Bonn tracks (right) with rotation. Symbol coding is used to distinguish between objects of different LC; magnetic stars and fast rotators are additionally highlighted by large squares and circles, respectively. In the lower three panels, different colours denote the morphologically peculiarly objects with very weak nitrogen lines (grey), and the stars whose predicted and observed [N] values differ by less (yellow) or more (green, orange) than 1σ. In the upper panels, the solid part of the tracks corresponds to the O-type phase (Teff ≥ 29 kK). The solar N abundance (from Asplund et al. 2005) is indicated by dotted 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.