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4
SO$_2$, silicate clouds, but no CH$_4$ detected in a warm Neptune
15NH3 in the atmosphere of a cool brown dwarf
Direct Evidence of Photochemistry in an Exoplanet Atmosphere
preprint published in 2022
The mass-loss rates of red supergiants at low metallicity: detection of rotational CO emission from two red supergiants in the Large Magellanic Cloud
article by Mikako Matsuura et al published 1 August 2016 in Monthly Notices of the Royal Astronomical Society
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