Young M dwarf flares exert greater chemical stress on primordial exo-Earth atmospheres than previous models, with potential for lasting changes in mixing ratios especially for low-abundance species.
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3 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 3representative citing papers
New X-ray flare detections from M dwarfs combined with literature data yield flare frequency constraints and an upper limit of 0.5-30 Myr on atmospheric loss times for habitable planets orbiting them.
Detection of GW Vir-type g-mode pulsations in Kn 61 central star gives period spacing 21.526 s and asteroseismic mass 0.551 solar masses consistent with evolutionary tracks.
citing papers explorer
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Stellar flare-driven evolution of primordial early exo-Earth atmospheres: Insights from a Young M Dwarf Flare model
Young M dwarf flares exert greater chemical stress on primordial exo-Earth atmospheres than previous models, with potential for lasting changes in mixing ratios especially for low-abundance species.
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Mapping the Landscape of M Dwarf X-ray Flares: New Discoveries in Context
New X-ray flare detections from M dwarfs combined with literature data yield flare frequency constraints and an upper limit of 0.5-30 Myr on atmospheric loss times for habitable planets orbiting them.
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Kepler Discovery of GW Vir Pulsations of the Central Star of Planetary Nebula Kn 61
Detection of GW Vir-type g-mode pulsations in Kn 61 central star gives period spacing 21.526 s and asteroseismic mass 0.551 solar masses consistent with evolutionary tracks.