The metal-rich atmosphere of the exo-Neptune HAT-P-26b
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DOI: 10.1093/mnras/stz789
Abstract: Transmission spectroscopy is enabling precise measurements of atmospheric H2O abundances for numerous giant exoplanets. For hot Jupiters, relating H2O abundances to metallicities provides a powerful probe of their formation conditions. However, metallicity measurements for Neptune-mass… read more here.
Keywords: hat 26b; neptune hat; exo neptune; h2o ... See more keywords