A Submillimeter Survey of CS Excitation in Protoplanetary Disks: Evidence of X-Ray-driven Sulfur Chemistry

The sulfur chemistry in protoplanetary disks influences the properties of nascent planets, including potential habitability. Although the inventory of sulfur molecules in disks has gradually increased over the last decade, CS is still the most commonly observed sulfur-bearing species, and it is expe...

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Autors principals:	Charles J. Law, Romane Le Gal, Karin I. Öberg, Ke Zhang, Yuri Aikawa, Sean M. Andrews, Jaehan Bae, Alice S. Booth, Gianni Cataldi, L. Ilsedore Cleeves, Feng Long, François Ménard, Chunhua Qi, Richard Teague, David J. Wilner
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2026-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	Astrochemistry Protoplanetary disks Planet formation
Accés en línia:	https://doi.org/10.3847/1538-4357/ae1fdf
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