Stellar laboratories - VIII. New Zr iv–vii, Xe iv–v, and Xe vii oscillator strengths and the Al, Zr, and Xe abundances in the hot white dwarfs G191−B2B and RE 0503−289

Free Access

Fig. 11

Open with DEXTER Download original image

Determined photospheric abundances of RE 0503−289 (cf. Fig. 10) compared with predictions for surface abundances of Karakas & Lugaro (2016, for an asymptotic giant branch (AGB) star with M_initial = 1.5 M_⊙, M_final = 0.585 M_⊙, metallicity Z = 0.014. [X/O] denotes the normalized log [(fraction of X/solar fraction of X)/(fraction of O/solar fraction of O)] mass ratio. The dashed green line indicates the solar ratio.

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.