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Magnetic Fields in the Bones of the Milky Way

Stars primarily form in galactic spiral arms within dense, filamentary molecular clouds. The largest and most elongated of these molecular clouds are referred to as “bones,” which are massive, velocity-coherent filaments (lengths ∼20 to >100 pc, widths ∼1–2 pc) that run approximately parallel and in...

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Autors principals: Ian W. Stephens, Simon Coudé, Philip C. Myers, Catherine Zucker, James M. Jackson, B.-G. Andersson, Rowan Smith, Archana Soam, Patricio Sanhueza, Taylor Hogge, Howard A. Smith, Giles Novak, Sarah Sadavoy, Thushara Pillai, Zhi-Yun Li, Leslie W. Looney, Koji Sugitani, Andrés E. Guzmán, Alyssa Goodman, Takayoshi Kusune, Miaomiao Zhang, Nicole Karnath, Jessy Marin
Format: Artigo
Idioma:Inglês
Publicat: IOP Publishing 2025-01-01
Col·lecció:The Astrophysical Journal
Matèries:
Star formation
Interstellar filaments
Interstellar magnetic fields
Young stellar objects
Polarimetry
Dust continuum emission
Accés en línia:https://doi.org/10.3847/1538-4357/ae08a8
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