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Paper: Strong Magnetic Fields in T Tauri Stars and Their Observational Consequences
Volume: 287, Galactic Star Formation Across the Stellar Mass Spectrum
Page: 292
Authors: Casali, M. M.
Abstract: Infrared Spectra of T Tauri stars show weak Fe I and strong OH lines compared to main sequence dwarfs of the same spectral type. These are interpreted as consistent with the presence of surface magnetic regions (starspots) with large fractional areas.
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