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Impact of photochemical hazes on the thermal structure of exoplanet atmospheres

Transit observations reveal that a significant population of the detected exoplanets has hazy atmospheres (Sing et al. 2016). Although the relative contribution of clouds and photochemical aerosols is not yet fully clarified, the impact of haze particles on the thermal structure could be significant, as such particles can efficiently scatter and absorb
Panayotis Lavvas, Anthony Arfaux
openaire   +1 more source

Possibilities for an Aerial Biosphere in Temperate Sub Neptune-Sized Exoplanet Atmospheres

Universe, 2021
Thomas M Evans   +2 more
exaly  

Can Isotopologues Be Used as Biosignature Gases in Exoplanet Atmospheres?

Life, 2023
Shuhei Ono   +2 more
exaly  

Phosphine as a Biosignature Gas in Exoplanet Atmospheres

Astrobiology, 2020
William Bains   +2 more
exaly  

Early Release Science of the exoplanet WASP-39b with JWST NIRSpec G395H

Nature, 2023
Thomas M Evans   +2 more
exaly  

Lightning and charge processes in brown dwarf and exoplanet atmospheres

Philosophical Transactions Series A, Mathematical, Physical, and Engineering Sciences, 2019
Paul Rimmer, Christiane Helling
exaly  

Structure and Evolution of an Exoplanet

Astronomy and Astrophysics Library, 2009
Franck Selsis   +2 more
exaly  

The Radiation Environment of Exoplanet Atmospheres

Challenges, 2014
Jeffrey Linsky, Linsky Jeffrey L
exaly  

Constraining Exoplanet Mass from Transmission Spectroscopy

Science, 2013
Sara Seager, Julien De Wit
exaly  

Gas Phase Chemistry of Cool Exoplanet Atmospheres: Insight from Laboratory Simulations

ACS Earth and Space Chemistry, 2019
Véronique Vuitton   +2 more
exaly  

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