Magnetic Effects and 3D Structure in Theoretical High-resolution Transmission Spectra of Ultrahot Jupiters: the Case of WASP-76b

High-resolution spectroscopy has allowed for unprecedented levels of atmospheric characterization, especially for the hottest gas-giant exoplanets known as ultrahot Jupiters (UHJs). High-resolution spectra are sensitive to 3D effects, making complex 3D atmospheric models important for interpreting d...

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Principais autores:	Hayley Beltz, Emily Rauscher, Eliza M.-R. Kempton, Isaac Malsky, Arjun B. Savel
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2023-01-01
coleção:	The Astronomical Journal
Assuntos:	Exoplanet atmospheres Hot Jupiters High resolution spectroscopy Transmission spectroscopy Atmospheric circulation Hydrodynamical simulations
Acesso em linha:	https://doi.org/10.3847/1538-3881/acd24d
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