The He I λ10830 Å line as a probe of winds and accretion in young stars in Lupus and Upper Scorpius

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Fig. D.1

He I λ10830 Å profiles of the Upper Scorpius sample, grouped by profile type. The profiles are normalised to the continuum level and rescaled between ± 1 for plotting. The black vertical dashes (at −88 km s⁻¹ and +126 km s⁻¹) mark photospheric absorption features (i.e Si I 10830.1 Å and NaI 10837.8 Å)

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