Unveiling the Atmosphere of HR 7672 B from the Near-infrared High-resolution Spectrum Using REACH/Subaru

Characterizing the atmospheres of exoplanets and brown dwarfs is crucial for understanding their atmospheric physics and chemistry, searching for biosignatures, and investigating their formation histories. Recent advances in observational techniques, combining adaptive optics with high-resolution sp...

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Detalles Bibliográficos

Autores principales:	Yui Kasagi, Yui Kawashima, Hajime Kawahara, Takayuki Kotani, Kento Masuda, Kyohoon Ahn, Olivier Guyon, Teruyuki Hirano, Nemanja Jovanovic, Masayuki Kuzuhara, Julien Lozi, Motohide Tamura, Taichi Uyama, Sebastien Vievard, Kenta Yoneta
Formato:	Artigo
Lenguaje:	Inglês
Publicado:	IOP Publishing 2025-01-01
Colección:	The Astronomical Journal
Materias:	Exoplanet atmospheres High resolution spectroscopy Brown dwarfs Exoplanets
Acceso en línea:	https://doi.org/10.3847/1538-3881/adf730
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