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Protosolar D-to-H Abundance and One Part per Billion PH3 in the Coldest Brown Dwarf

The coldest Y spectral type brown dwarfs are similar in mass and temperature to cool and warm (∼200–400 K) giant exoplanets. We can therefore use their atmospheres as proxies for planetary atmospheres, testing our understanding of physics and chemistry for these complex, cool worlds. At these cold t...

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Hoofdauteurs: Melanie J. Rowland, Caroline V. Morley, Brittany E. Miles, Genaro Suarez, Jacqueline K. Faherty, Andrew J. Skemer, Samuel A. Beiler, Michael R. Line, Gordon L. Bjoraker, Jonathan J. Fortney, Johanna M. Vos, Sherelyn Alejandro Merchan, Mark Marley, Ben Burningham, Richard Freedman, Ehsan Gharib-Nezhad, Natasha Batalha, Roxana Lupu, Channon Visscher, Adam C. Schneider, T. R. Geballe, Aarynn Carter, Katelyn Allers, James Mang, Dániel Apai, Mary Anne Limbach, Mikayla J. Wilson
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: IOP Publishing 2024-01-01
Reeks:The Astrophysical Journal Letters
Onderwerpen:
Planetary atmospheres
Brown dwarfs
Y dwarfs
Exoplanet atmospheres
Exoplanet atmospheric composition
Online toegang:https://doi.org/10.3847/2041-8213/ad9744
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