A consistent analysis of 67 T Tauri stars finds typical magnetospheric truncation radii near 2.8 stellar radii, about half the standard 5 stellar radius assumption, with up to half of accretion luminosity emitted in the UV.
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The ODYSSEUS Survey. Characterizing magnetospheric geometries and hotspot structures in T Tauri stars
A consistent analysis of 67 T Tauri stars finds typical magnetospheric truncation radii near 2.8 stellar radii, about half the standard 5 stellar radius assumption, with up to half of accretion luminosity emitted in the UV.