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Asymmetric Temperature Variations In Protoplanetary Disks. I. Linear Theory, Corotating Spirals, and Ring Formation

Protoplanetary disks can exhibit asymmetric temperature variations due to phenomena such as shadows cast by the inner disk or localized heating by young planets. We investigate the disk features induced by these asymmetric temperature variations. We find that spirals are initially excited, and then...

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Bibliografiset tiedot
Päätekijät: Zhaohuan Zhu, Shangjia Zhang, Ted M. Johnson
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: IOP Publishing 2025-01-01
Sarja:The Astrophysical Journal
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Linkit:https://doi.org/10.3847/1538-4357/adae0d
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