Fig. 8.

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Activity index () vs. accretion rate (log Ṁ) for selected sources. Red filled circles indicate accretion rates derived from the width of Hα at 10% of the peak by the Gaia-ESO survey (Lanzafame et al. 2015, and references therein). Blue filled circles indicate accretion rates derived from the excess continuum emission (see, e.g. Manara et al. 2015). See Table 2 for the sources of the accretion rate estimates.
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