Fig. 2
Comparison of projected rotational velocities estimated using the FT and PF methodologies. The upper figure is for the narrower lined stars (line set 1), whilst the lower figure is for the broader lined (line set 2) sample. Also shown are the results of the simulation – crosses: He i 4713 Å; asterisks: Si iii 4552 Å or He i 4387 Å.
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