SOFIA Observations of 30 Doradus. II. Magnetic Fields and Large-scale Gas Kinematics

SOFIA Observations of 30 Doradus. II. Magnetic Fields and Large-scale Gas Kinematics

The heart of the Large Magellanic Cloud, 30 Doradus, is a complex region with a clear core-halo structure. Feedback from the stellar cluster R136 has been shown to be the main source of energy creating multiple parsec-scale expanding-shells in the outer region, and carving a nebula core in the proxi...

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Bibliographic Details
Main Authors: Le Ngoc Tram, Lars Bonne, Yue Hu, Enrique Lopez-Rodriguez, Jordan A. Guerra, Pierre Lesaffre, Antoine Gusdorf, Thiem Hoang, Min-Young Lee, Alex Lazarian, B-G Andersson, Simon Coudé, Archana Soam, William D. Vacca, Hyeseung Lee, Michael Gordon
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Interstellar dust
Interstellar dust extinction
Star formation
Interstellar magnetic fields
Magnetic fields
Interstellar dynamics
Online Access:https://doi.org/10.3847/1538-4357/acaab0

Internet

https://doi.org/10.3847/1538-4357/acaab0

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