Fig. 7
Same as Fig. 3, but for HD 45 314. Typical uncertainties on the EWs are 0.50, 0.25, and 0.20 Å for the Hα, Hβ, and He i λ 5876 lines respectively. We have also included the EW(Hα) measurement of Silaj et al. (2010). The second Coralie spectrum was taken simultaneously with the XMM-Newton observation discussed by Rauw et al. (2013).
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