HCN and C2H2 in the Atmosphere of a T8.5+T9 Brown Dwarf Binary

HCN and C2H2 in the Atmosphere of a T8.5+T9 Brown Dwarf Binary

T-type brown dwarfs present an opportunity to explore atmospheres teeming with molecules such as H _2 O, CH _4 , and NH _3 , which exhibit a wealth of absorption features in the mid-infrared. With JWST, we can finally explore this chemistry in detail, including for the coldest brown dwarfs that were...

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Detalhes bibliográficos
Principais autores: Elisabeth C. Matthews, Paul Mollière, Helena Kühnle, Polychronis Patapis, Niall Whiteford, Matthias Samland, Pierre-Olivier Lagage, Rens Waters, Shang-Min Tsai, Kevin Zahnle, Manuel Guedel, Thomas Henning, Bart Vandenbussche, Olivier Absil, Ioannis Argyriou, David Barrado, Alain Coulais, Adrian M. Glauser, Goran Olofsson, John P. Pye, Daniel Rouan, Pierre Royer, Ewine F. van Dishoeck, T. P. Ray, Göran Östlin
Formato: Artigo
Idioma:English
Publicado em: IOP Publishing 2025-01-01
coleção:The Astrophysical Journal Letters
Assuntos:
Brown dwarfs
T dwarfs
Stellar atmospheres
Exoplanet atmospheres
Extrasolar gaseous giant planets
Acesso em linha:https://doi.org/10.3847/2041-8213/adb4ec

Internet

https://doi.org/10.3847/2041-8213/adb4ec

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