The Protostars in Orion: Characterizing the Properties of Their Magnetized Envelopes

The Protostars in Orion: Characterizing the Properties of Their Magnetized Envelopes

We present a study connecting the physical properties of protostellar envelopes to the morphology of the envelope-scale magnetic field. We used the Atacama Large Millimeter/submillimeter Array (ALMA) polarization observations of 61 young protostars at 0.87 mm on ~400–3000 au scales from the B -field...

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Bibliographic Details
Main Authors: Bo Huang, Josep M. Girart, Ian W. Stephens, Manuel Fernández López, Philip C. Myers, Qizhou Zhang, John J. Tobin, Paulo Cortes, Nadia M. Murillo, Sarah Sadavoy, Hector G. Arce, John M. Carpenter, Woojin Kwon, Valentin J. M. Le Gouellec, Zhi-Yun Li, Leslie W. Looney, Tom Megeath, Erin G. Cox, Nicole Karnath, Dominique Segura-Cox
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Star formation
Star forming regions
Magnetic fields
Interstellar magnetic fields
Circumstellar envelopes
Circumstellar disks
Online Access:https://doi.org/10.3847/1538-4357/ad9ea4
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https://doi.org/10.3847/1538-4357/ad9ea4

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