MHD Simulations of Strongly Magnetized H ii Region Evolution: Evidence for Ionized Gas Filamentation

Recent James Webb Space Telescope observations of H ii  regions in the Central Molecular Zone (CMZ) have shown a highly filamentary morphology distinct from H ii  regions in other parts of the Galaxy. We present magnetohydrodynamic (MHD) simulations of strongly magnetized (plasma- β  ≪ 1) H ii  regi...

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Hlavní autoři:	Samuel Crowe, Yisheng Tu, Zhi-Yun Li, Jeong-Gyu Kim, John Bally
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2026-01-01
Edice:	The Astrophysical Journal
Témata:	H II regions Galactic center Radiative magnetohydrodynamics Magnetohydrodynamical simulations Interstellar filaments Star formation
On-line přístup:	https://doi.org/10.3847/1538-4357/ae4bd7
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