Fig. E.30
The temperature of VFTS 506 (ON2 V((n))((f*))) is based on the lines N iii λ4634/4640, N iv λ4058, and N v λ4604/4620. The model temperature is slightly too low. Ṁ is based on the line shape of He ii λ4686. log g might be a bit higher, because the observations are a bit broader than the model. The star is fast rotating. N-abundance is between normal and enriched.
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.