Fig. 18
Final models for all our sample considering solar abundances (red). Re-computed models using ɛCNO from Martins et al. (2015a) are in dashed blue. IUE data are in black. We indicate, right above each spectrum, whether ɛCNO is a determination from Martins et al. (2015a) or an adoption based on their results (see text for details). We note that the highest effects in C IV λλ1548,1551 are due to the adopted ɛCNO.
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