Clouds and hazes are important throughout our solar system and in the atmospheres of brown dwarfs and extrasolar giant planets. Among the brown dwarfs, clouds control the colors and spectra of the L-dwarfs; the disappearance of clouds helps herald the arrival of the T-dwarfs. The structure and composition of clouds will be among the first remote-sensing results from the direct detection of extrasolar giant planets
This PhD thesis presents work on the atmospheres of both brown dwarfs and exoplanets from an observe...
Brown dwarfs have cool atmospheres with the temperatures of giant planets. Their atmospheres are coo...
The precipitation of cloud particles in brown dwarf and exoplanet atmospheres establishes an ongoing...
Clouds and hazes are commonplace in the atmospheres of solar system planets and are likely ubiquitou...
The formation of clouds significantly alters the spectra of cool substellar atmospheres from terrest...
Accepted in ApJL, comments welcomeThe admitted, conventional scenario to explain the complex spectra...
Brown dwarfs are substellar objects intermediate between stars and giant planets. Currently detected...
The properties of clouds is perhaps one of the most crucial factors for correctly interpreting the o...
International audienceThe admitted, conventional scenario to explain the complex spectral evolution ...
<p>Observational evidence has suggested that there is active meteorology in the atmospheres of brown...
The admitted, conventional scenario to explain the complex spectral evolution of brown dwarfs (BDs) ...
Clouds of metal-bearing condensates play a critical role in shaping the emergent spectral energy dis...
The formation of clouds affects brown dwarf and planetary atmospheres of nearly all effective temper...
We developed a simple, physical and self-consistent cloud model for brown dwarfs and young giant exo...
Clouds of sand can consolidate, develop and vanish in a few extraterrestrial atmospheres. Another ga...
This PhD thesis presents work on the atmospheres of both brown dwarfs and exoplanets from an observe...
Brown dwarfs have cool atmospheres with the temperatures of giant planets. Their atmospheres are coo...
The precipitation of cloud particles in brown dwarf and exoplanet atmospheres establishes an ongoing...
Clouds and hazes are commonplace in the atmospheres of solar system planets and are likely ubiquitou...
The formation of clouds significantly alters the spectra of cool substellar atmospheres from terrest...
Accepted in ApJL, comments welcomeThe admitted, conventional scenario to explain the complex spectra...
Brown dwarfs are substellar objects intermediate between stars and giant planets. Currently detected...
The properties of clouds is perhaps one of the most crucial factors for correctly interpreting the o...
International audienceThe admitted, conventional scenario to explain the complex spectral evolution ...
<p>Observational evidence has suggested that there is active meteorology in the atmospheres of brown...
The admitted, conventional scenario to explain the complex spectral evolution of brown dwarfs (BDs) ...
Clouds of metal-bearing condensates play a critical role in shaping the emergent spectral energy dis...
The formation of clouds affects brown dwarf and planetary atmospheres of nearly all effective temper...
We developed a simple, physical and self-consistent cloud model for brown dwarfs and young giant exo...
Clouds of sand can consolidate, develop and vanish in a few extraterrestrial atmospheres. Another ga...
This PhD thesis presents work on the atmospheres of both brown dwarfs and exoplanets from an observe...
Brown dwarfs have cool atmospheres with the temperatures of giant planets. Their atmospheres are coo...
The precipitation of cloud particles in brown dwarf and exoplanet atmospheres establishes an ongoing...