Fig. A.9

Cross-correlation function of the HERMES spectrum of WDS 19255+0307Aa,Ab (obtained at JD 2 455 657.742) with a F0V template. Component Aa shows a rotationally broadened profile with Vrsini = 84 km s-1, and component Ab is visible as a weak Gaussian (at Vr(Ab) = –37.70 km s-1) superimposed on the rotationally broadened profile (centred on Vr(Aa) = –26.68 km s-1). Similar profiles have been observed over several consecutive nights.
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