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ACES: The Magnetic Field in Large Filaments in the Galactic Center

The Galactic center (GC) is an extreme region of the Milky Way that is host to a complex set of thermal and nonthermal structures. In particular, the GC contains high-density gas and dust that is collectively referred to as the Central Molecular Zone (CMZ). In this work, we study a subset of HNCO fi...

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Hoofdauteurs: Dylan M. Paré, Zi-Xuan Feng, Yue Hu, Maya A. Petkova, Jack Sullivan, Robin G. Tress, Cara Battersby, Janik Karoly, Alex Lazarian, Dani Lipman, Xing Pan, Marco Donati, Mattia C. Sormani, John Bally, Ashley T. Barnes, Natalie O. Butterfield, Laura Colzi, Christoph Federrath, Pablo Garcia, Adam Ginsburg, Savannah R. Gramze, Anika Schmiedeke, Christian Henkel, Jonathan D. Henshaw, Paul T. Ho, Pei-Ying Hsieh, Izaskun Jimenez-Serra, Ralf S. Klessen, J. M. Diederik Kruijssen, Steven N. Longmore, Xing Lu, Elisabeth A.C. Mills, Álvaro Sánchez-Monge, Daniel L. Walker, Jennifer Wallace, Qizhou Zhang
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: IOP Publishing 2026-01-01
Reeks:The Astrophysical Journal
Onderwerpen:
Interstellar medium
Galactic center
Interstellar magnetic fields
Dense interstellar clouds
Interstellar filaments
Polarimetry
Online toegang:https://doi.org/10.3847/1538-4357/ae22ce
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