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Fig. 12

image

Photosphere-subtracted Hα (top) and Hβ (bottom) spectra observed with HIRES/Keck (for various epochs) and X-shooter (corresponding to the time when the accretion rate and the stellar properties were estimated; Manara et al., in prep.). Zero levels for flux and radial velocity are marked by dotted lines. A rotationally-broadened template photosphere has been subtracted to show absorption and emission features.

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