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...

ver descrição completa

Detalhes bibliográficos

Principais autores:	Samuel Crowe, Yisheng Tu, Zhi-Yun Li, Jeong-Gyu Kim, John Bally
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2026-01-01
Colecção:	The Astrophysical Journal
Assuntos:	H II regions Galactic center Radiative magnetohydrodynamics Magnetohydrodynamical simulations Interstellar filaments Star formation
Acesso em linha:	https://doi.org/10.3847/1538-4357/ae4bd7
Tags:	Adicionar Tag Sem tags, seja o primeiro a adicionar uma tag!