Cosmic rays accelerated at a T Tauri star's accretion shock can raise disk ionization far above the Galactic background and extend the region where the magneto-rotational instability operates, possibly creating a self-regulating accretion cycle.
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Impact of Cosmic-Ray Feedback on Accretion and Chemistry in Circumstellar Disks
Cosmic rays accelerated at a T Tauri star's accretion shock can raise disk ionization far above the Galactic background and extend the region where the magneto-rotational instability operates, possibly creating a self-regulating accretion cycle.