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...

Descripció completa

Dades bibliogràfiques

Autors principals:	Hayley Beltz, Emily Rauscher, Eliza M.-R. Kempton, Isaac Malsky, Arjun B. Savel
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2023-01-01
Col·lecció:	The Astronomical Journal
Matèries:	Exoplanet atmospheres Hot Jupiters High resolution spectroscopy Transmission spectroscopy Atmospheric circulation Hydrodynamical simulations
Accés en línia:	https://doi.org/10.3847/1538-3881/acd24d
Etiquetes:	Afegir etiqueta Sense etiquetes, Sigues el primer a etiquetar aquest registre!