Kinematic evidence of magnetospheric accretion for Herbig Ae stars with JWST NIRSpec

Open Access

Fig. 8.

Line profiles of Br₁₁ and Br₆, respectively shown as solid and dashed black lines. The green solid line shows the line profile ratio $\frac{{Br}_{10}}{{Br}_{6}}$ $\frac{\mathrm{Br}_{10}}{\mathrm{Br}_{6}}$ . Line profile ratio uncertainties are shown as green error bars.

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