Stellar laboratories - VI. New Mo iv–vii oscillator strengths and the molybdenum abundance in the hot white dwarfs G191−B2B and RE 0503−289

Free Access

Fig. 16

Open with DEXTER Download original image

Like Fig. 12 for G191−B2B. The thick red and thin blue spectra are calculated from models with photospheric Mo abundances of 5.3 × 10^-6 and 5.3 × 10^-7 (mass fractions, about 1000 and 100 times the solar value), respectively.

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.