Modeling Circumstellar Gas Emission around a White Dwarf Using cloudy

The chemical composition of an extrasolar planet is fundamental to its formation, evolution, and habitability. In this study, we explore a new way to measure the chemical composition of the building blocks of extrasolar planets by measuring the gas composition of the disrupted planetesimals around w...

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Detalles Bibliográficos

Autores principales:	Siyi Xu, Sherry Yeh, Laura. K. Rogers, Amy Steele, Erik Dennihy, Alexandra E. Doyle, P. Dufour, Beth L. Klein, Christopher J. Manser, Carl Melis, Tinggui Wang, Alycia J. Weinberger
Formato:	Artigo
Lenguaje:	Inglês
Publicado:	IOP Publishing 2024-01-01
Colección:	The Astronomical Journal
Materias:	Circumstellar gas Chemical abundances Debris disks Planetesimals Extrasolar rocky planets White dwarf stars
Acceso en línea:	https://doi.org/10.3847/1538-3881/ad3737
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