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Helical Magnetic Field in the Acceleration–Collimation Zone of the M87 Jet

Relativistic jets from supermassive black holes are expected to be magnetically launched and guided, with magnetic energy systematically converted to bulk kinetic energy throughout an extended acceleration–collimation zone (ACZ). A key prediction of magnetohydrodynamic (MHD) models is a transition f...

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Guardat en:
Autors principals: Jongho Park, Kazuya Takahashi, Kenji Toma, Kazuhiro Hada, Masanori Nakamura, Hung-Yi Pu, Keiichi Asada, Paul T. P. Ho, Motoki Kino, Tomohisa Kawashima, Minchul Kam, Kunwoo Yi, Ilje Cho
Format: Artigo
Idioma:Inglês
Publicat: IOP Publishing 2026-01-01
Col·lecció:The Astrophysical Journal Letters
Matèries:
Active galactic nuclei
Relativistic jets
Very long baseline interferometry
Polarimetry
Magnetohydrodynamics
Magnetic fields
Accés en línia:https://doi.org/10.3847/2041-8213/ae1ffe
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