Water- and metal-rich atmospheres on compact hot mini-Neptunes lose mass more slowly than H/He cases at high enrichment levels due to enhanced cooling and higher mean molecular weight.
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Numerical model of fast electron energy loss in H2 finds 11% of energy to direct ro-vibrational excitation and 1.5-2 times higher yields for high-vibrational states via electronic cascading than earlier Monte Carlo calculations.
citing papers explorer
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Escape of Water- and Metal-enriched Atmospheres from compact Hot mini-Neptunes with CHAIN
Water- and metal-rich atmospheres on compact hot mini-Neptunes lose mass more slowly than H/He cases at high enrichment levels due to enhanced cooling and higher mean molecular weight.
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Numerical model of fast electron energy deposition in interstellar molecular gas
Numerical model of fast electron energy loss in H2 finds 11% of energy to direct ro-vibrational excitation and 1.5-2 times higher yields for high-vibrational states via electronic cascading than earlier Monte Carlo calculations.