For most of 47 classical T Tauri stars, the fastness parameter is below equilibrium, implying active angular momentum loss and dynamic star-disk interaction.
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The ODYSSEUS Survey. Using accretion and stellar rotation to reveal the star-disk connection in T Tauri stars
For most of 47 classical T Tauri stars, the fastness parameter is below equilibrium, implying active angular momentum loss and dynamic star-disk interaction.