Fig. 11
Relative strengths of Mo lines calculated from our stellar-atmosphere model of RE 0503−289. Top graph: Mo iv–vii lines, the four most prominent are Mo vi lines that were identified by Werner et al. (2012b) are marked. Graphs 2 to 5 (from top to bottom): lines of individual Mo iv–vii ions (intensities reduced by a factor of 0.22 compared to the top graph), respectively.
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