The First Estimation of the Ambipolar Diffusivity Coefficient from Multi-scale Observations of the Class 0/I Protostar, HOPS-370

Protostars are born in magnetized environments. As a consequence, the formation of protostellar disks can be suppressed by the magnetic field, efficiently removing the angular momentum of the infalling material. Nonideal MHD effects are proposed as one way to allow protostellar disks to form. Thus,...

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Detalhes bibliográficos

Principais autores:	Travis J. Thieme, Shih-Ping Lai, Yueh-Ning Lee, Sheng-Jun Lin, Hsi-Wei Yen
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2024-01-01
coleção:	The Astrophysical Journal
Assuntos:	Circumstellar disks Observational astronomy Radio astronomy Star formation Protostars Young stellar objects
Acesso em linha:	https://doi.org/10.3847/1538-4357/ad4297
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