Magnetic fields in six of nine T-Tauri stars show rotationally modulated variability that evolves in strength and spatial distribution over year-long baselines, with magnetic filling factors larger than temperature-derived spot areas.
P., G¨ udel, M., & Lammer, H
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Young sub-Neptunes transition from core-powered bolometric escape to photoevaporative escape at smaller radii for lower-mass and more irradiated planets, with self-consistent simulations yielding combined mass-loss rates and analytic transition scalings.
Observational analysis of 85 FGK stars yields X-ray luminosity and temperature relations with age, confirming t^{-1.5} decay in soft band while noting increased scatter in harder band at older ages.
citing papers explorer
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Rotational Modulation and Long-Term Variability of Magnetic Fields in T-Tauri Stars with IGRINS
Magnetic fields in six of nine T-Tauri stars show rotationally modulated variability that evolves in strength and spatial distribution over year-long baselines, with magnetic filling factors larger than temperature-derived spot areas.
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Characterizing the bolometric-photoevaporative transition in young sub-Neptunes with radiation-hydrodynamic simulations
Young sub-Neptunes transition from core-powered bolometric escape to photoevaporative escape at smaller radii for lower-mass and more irradiated planets, with self-consistent simulations yielding combined mass-loss rates and analytic transition scalings.
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X-ray Emission and Stellar Ages of Sun-Like Stars
Observational analysis of 85 FGK stars yields X-ray luminosity and temperature relations with age, confirming t^{-1.5} decay in soft band while noting increased scatter in harder band at older ages.