The Hourglass-shaped Magnetic Fields and Dust Filaments in the HH 211 Protostellar Envelope

Magnetic fields influence the structure and evolution of protostellar systems; thus, understanding their role is essential for probing the earliest stages of star formation. We present Atacama Large Millimeter/submillimeter Array Band 3 and 6 polarized continuum observations at ∼0 $\mathop{.}\limits...

Fuld beskrivelse

Bibliografiske detaljer

Principais autores:	Youngwoo Choi, Woojin Kwon, Leslie W. Looney, Ian W. Stephens, Zhi-Yun Li, Floris F. S. van der Tak, John J. Tobin
Format:	Artigo
Sprog:	Inglês
Udgivet:	IOP Publishing 2025-01-01
Serier:	The Astrophysical Journal
Fag:	Observational astronomy Young stellar objects Protostars Radio astronomy Interstellar magnetic fields Star formation
Online adgang:	https://doi.org/10.3847/1538-4357/ae0710
Tags:	Tilføj Tag Ingen Tags, Vær først til at tagge denne postø!