Chemical abundances of fast-rotating massive stars - I. Description of the methods and individual results

Free Access

Fig. E.2

Open with DEXTER Download original image

Same as Fig. E.1, but for HD 13268 (ON8.5IIIn; vsin i = 301 km s^-1). He i lines are generally well fitted, except He i 5876. Some nitrogen lines, e.g. N iii 4634–4643, are not perfectly fitted.

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.