The apparent excess of T Tauri binaries at 10-100 au disappears when surveys are limited by spectral type instead of magnitude, because close binaries clear their dusty disks faster and are over-represented in brightness-limited samples.
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New Insights into the T Tauri Binary Separation Distribution
The apparent excess of T Tauri binaries at 10-100 au disappears when surveys are limited by spectral type instead of magnitude, because close binaries clear their dusty disks faster and are over-represented in brightness-limited samples.