Extended Data Fig. 1: [O I] λ6300 line profiles of TW Hya.
From: High-resolution [O I] line spectral mapping of TW Hya supportive of a magnetothermal wind
a, Distribution of the [O I] λ6300 line centroids of TW Hya and. These spectra are taken with ESPaDOnS (gray color filled histogram), FEROS or HARPS (maroon line filled histogram), and UVES or HIRES (olive open histogram). The numbers of the used spectra from individual instruments are shown in the figure. b, Comparisons of the [O I] λ6300 line profiles of TW Hya. For the comparisons, the centroids of the lines have been shifted to the mean centroid (-0.8 km s−1) and the spectral resolutions have been degraded to 40000. The colors are the same as in a.
