Atmospheric Mass Loss from TOI-1259 A b, a Gas Giant Planet with a White Dwarf Companion

The lack of close-in Neptune-mass exoplanets evident in transit surveys has largely been attributed to either photoevaporative mass loss or high-eccentricity migration. To distinguish between these two possibilities, we investigate the origins of TOI-1259 A b, a Saturn-mass (0.4 M _J , 1.0 R _J ) ex...

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Autors principals:	Morgan Saidel, Shreyas Vissapragada, Jessica Spake, Heather A. Knutson, Dion Linssen, Michael Zhang, Michael Greklek-McKeon, Jorge Pérez-González, Antonija Oklopčić
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2025-01-01
Col·lecció:	The Astronomical Journal
Matèries:	Exoplanet evolution Exoplanets Exoplanet atmospheres Exoplanet astronomy Planetary atmospheres Extrasolar gaseous planets
Accés en línia:	https://doi.org/10.3847/1538-3881/ada49f
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