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. 16

Gaussian area, in units of km s⁻¹ × normalised flux units, versus log(L_acc/L_*) of the emission features in pure emission, P Cygni, inverse P Cygni and combination profile types separated by star-forming region. The line of best fit for all datapoints is marked in grey, with a linear fit for Lupus and Upper Sco in black and green, respectively.

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