Stellar winds from young weak-lined T Tauri stars compress exoplanet magnetospheres to sizes significantly smaller than Earth's, with sizes increasing as stellar activity decays with age.
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Combined TESS-CHEOPS data on 5620 flares shows ED-based FFDs follow power laws but bolometric-energy FFDs are best described by a truncated power law with break at 1.8e35 erg, with low-energy flattening attributed to detection biases rather than intrinsic lognormal behavior.
citing papers explorer
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Interaction between Winds from Weak-lined T Tauri Stars with Exoplanetary Magnetospheres
Stellar winds from young weak-lined T Tauri stars compress exoplanet magnetospheres to sizes significantly smaller than Earth's, with sizes increasing as stellar activity decays with age.
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Extending TESS flare frequency distributions with CHEOPS: Power-law versus lognormal
Combined TESS-CHEOPS data on 5620 flares shows ED-based FFDs follow power laws but bolometric-energy FFDs are best described by a truncated power law with break at 1.8e35 erg, with low-energy flattening attributed to detection biases rather than intrinsic lognormal behavior.