Fig. 1.

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log fc- and log fp-values for the luminosity class III–V primaries in the SB1 (black symbols) and SB1* (red symbols) systems. Upper limits are indicated as downward triangles. Filled symbols denote systems that have eccentricities within 2-σ of zero. Also shown are the upper limits for synchronous rotation assuming that the secondaries contribute negligible flux (dashed black line) and 20% (dashed blue line) of the total flux. The red dashed line in the upper panel shows the position at period P that a “typical” B-type star with radius 8 R⊙ and v sin i = 150 km s−1 would have for synchronisation. Also shown is the typical error estimate.
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