Predicting Cloud Conditions in Substellar Mass Objects Using Ultracool Dwarf Companions

Predicting Cloud Conditions in Substellar Mass Objects Using Ultracool Dwarf Companions

We present results from conducting a theoretical chemical analysis of a sample of benchmark companion brown dwarfs whose primary star is of type F, G, or K. We summarize the entire known sample of these types of companion systems, termed “compositional benchmarks,” that are present in the literature...

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Bibliographic Details
Main Authors: Emily Calamari, Jacqueline K. Faherty, Channon Visscher, Marina E. Gemma, Ben Burningham, Austin Rothermich
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Brown dwarfs
Main sequence stars
Wide binary stars
Exoplanet atmospheres
Atmospheric clouds
Astrochemistry
Online Access:https://doi.org/10.3847/1538-4357/ad1f6d

Internet

https://doi.org/10.3847/1538-4357/ad1f6d

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