Protosolar D-to-H abundance and one part-per-billion PH$_{3}$ in the coldest brown dwarf

Documenti analoghi

• The Sonora Substellar Atmosphere Models. IV. Elf Owl: Atmospheric Mixing and Chemical Disequilibrium with Varying Metallicity and C/O Ratios
  di: Mukherjee, Sagnick, et al.
  Pubblicazione: (2024)
• The Sonora Substellar Atmosphere Models. III. Diamondback: Atmospheric Properties, Spectra, and Evolution for Warm Cloudy Substellar Objects
  di: Morley, Caroline V., et al.
  Pubblicazione: (2024)
• A Tale of Two Molecules: The Underprediction of CO$_2$ and Overprediction of PH$_3$ in Late T and Y Dwarf Atmospheric Models
  di: Beiler, Samuel A., et al.
  Pubblicazione: (2024)
• A Comprehensive Atmospheric Retrieval Analysis of 22 James Webb Space Telescope Spectral Energy Distributions of Cool Brown Dwarfs
  di: Kothari, Harshil, et al.
  Pubblicazione: (2026)
• Predicting Cloud Conditions in Substellar Mass Objects Using Ultracool Dwarf Companions
  di: Calamari, Emily, et al.
  Pubblicazione: (2024)