Disentangling CO Chemistry in a Protoplanetary Disk Using Explanatory Machine-learning Techniques

Disentangling CO Chemistry in a Protoplanetary Disk Using Explanatory Machine-learning Techniques

Molecular abundances in protoplanetary disks are highly sensitive to the local physical conditions, including gas temperature, gas density, radiation field, and dust properties. Often multiple factors are intertwined, impacting the abundances of both simple and complex species. We present a new appr...

Detaylı Bibliyografya
Asıl Yazarlar:	Amina Diop, L. Ilsedore Cleeves, Dana E. Anderson, Jamila Pegues, Adele Plunkett
Materyal Türü:	Makale
Dil:	English
Baskı/Yayın Bilgisi:	IOP Publishing 2024-01-01
Seri Bilgileri:	The Astrophysical Journal
Konular:	Protoplanetary disks Astrochemistry Chemical reaction network models Regression
Online Erişim:	https://doi.org/10.3847/1538-4357/ad11ed

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