Exoplanet HD 209458b: Inflated Hydrogen Atmosphere but No Sign of Evaporation [PDF]
, 2007 Lotfi Ben‐Jaffel
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Tropical Cyclones on Tidally Locked Rocky Planets: Dependence on Rotation Period
The Astrophysical JournalTropical cyclones occur over the Earth’s tropical oceans, with characteristic genesis regions and tracks tied to the warm ocean surface that provide energy to sustain these storms.
Valeria Garcia +3 more
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A TEMPERATURE AND ABUNDANCE RETRIEVAL METHOD FOR EXOPLANET ATMOSPHERES [PDF]
, 2009 Nikku Madhusudhan, S. Seager
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Exoplanet atmospheres: A theoretical outlook [PDF]
Proceedings of the International Astronomical Union, 2010 AbstractWith over two dozen exoplanet atmospheres observed today, the field of exoplanet atmospheres is solidly established. The highlights of exoplanet atmosphere studies include: detection of molecular spectral features; constraints on atmospheric vertical temperature structure; detection of day-night temperature gradients; and a new numerical ...
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LIGHT SCATTERING FROM EXOPLANET OCEANS AND ATMOSPHERES [PDF]
, 2010 Michael E. Zugger +4 more
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The Astrophysical JournalInhomogeneous cloud formation and wavelength-dependent phenomena are expected to shape hot Jupiter atmospheres. We present a general circulation model with multiwavelength “picket fence” radiative transfer and radiatively active, temperature-dependent ...
Isaac Malsky +7 more
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Ex(o)plain: Subgroup-Level Analysis of Exoplanet Atmospheric Parameters
IEEE AccessDeep learning has been shown to be a valuable tool in astrophysics. In the field of exoplanetary science, deep learning-based approaches are being used extensively to automate the characterization of exoplanet atmospheres, reducing computational costs ...
Alkis Koudounas +2 more
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Atmospheric escape from exoplanets: recent observations and theoretical models [PDF]
arXivThe review aims to give an overview of atmospheric escape processes from exoplanets. I briefly discuss the physics of various escape processes responsible for atmospheric escape across different types of exoplanets. Transmission spectroscopy is one of the major workhorses to observe the escaping atmosphere from exoplanets. I discuss recent observations
arxiv
Atmospheric Mass Loss from TOI-1259 A b, a Gas Giant Planet with a White Dwarf Companion
The Astronomical JournalThe lack of close-in Neptune-mass exoplanets evident in transit surveys has largely been attributed to either photoevaporative mass loss or high-eccentricity migration.
Morgan Saidel +8 more
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The upper atmosphere of the exoplanet HD209458b revealed by the sodium D lines: temperature-pressure profile, ionization layer and thermosphere (Corrigendum) [PDF]
, 2011 A. Vidal‐Madjar +9 more
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