Fig. 3.
Measured primary RVs for simulated spectra of one single B2 V star, and SB2 binary systems with a B2 V primary and six different mass ratios as indicated in the legend. A rotational velocity of v sini = 200 km s−1 is assumed for all stars. The horizontal axis gives the assumed RV difference between the two components. The dashed line indicates the true velocity of the primary star.
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