Resolving the FU Orionis System with ALMA: Interacting Twin Disks?

FU Orionis objects are low-mass pre-main sequence stars characterized by dramatic outbursts several magnitudes in brightness. These outbursts are linked to episodic accretion events in which stars gain a significant portion of their mass. The physical processes behind these accretion events are not...

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Detalles Bibliográficos
Autores principales: Perez, Sebastian, Hales, Antonio, Liu, Hauyu Baobab, Zhu, Zhaohuan, Casassus, Simon, Williams, Jonathan, Zurlo, Alice, Cuello, Nicolas, Cieza, Lucas, Principe, David
Formato: Artículo (Article)
Idioma:Inglés (English)
Publicado: 2025
Materias:
Stellar accretion disks
Star formation
FU Orionis stars
Circumstellar gas
Submillimeter astronomy
Millimeter astronomy
Acceso en línea:https://repositorio.uc.cl/handle/11534/100659

Internet

https://repositorio.uc.cl/handle/11534/100659

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