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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3 Pith papers cite this work. Polarity classification is still indexing.
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Observational study of 290 exoplanet-host stars finds higher C, O, S, Fe, Ni abundances in giant-planet hosts than small-planet hosts, with C/O ratios, hot/warm differences, and mass correlations that vary by subpopulation.
Including tidal and centrifugal gravity corrections increases retrieved molecular abundances in transmission spectra retrievals for WASP-12b (HST) and WASP-39b (JWST).
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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Chemical Abundances of the Bioessential Elements C, O and S, and the Refractory Elements Fe and Ni, in Solar-type Exoplanet-hosting Stars from HARPS North and South
Observational study of 290 exoplanet-host stars finds higher C, O, S, Fe, Ni abundances in giant-planet hosts than small-planet hosts, with C/O ratios, hot/warm differences, and mass correlations that vary by subpopulation.
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Effect of tidal gravity and planetary rotation on the retrieved atmospheric abundances of close-in exoplanets
Including tidal and centrifugal gravity corrections increases retrieved molecular abundances in transmission spectra retrievals for WASP-12b (HST) and WASP-39b (JWST).