Codice QR

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...

Descrizione completa

Salvato in:
Autori principali: Samuel Crowe, Yisheng Tu, Zhi-Yun Li, Jeong-Gyu Kim, John Bally
Natura: Artigo
Lingua:Inglês
Pubblicazione: IOP Publishing 2026-01-01
Serie:The Astrophysical Journal
Soggetti:
H II regions
Galactic center
Radiative magnetohydrodynamics
Magnetohydrodynamical simulations
Interstellar filaments
Star formation
Accesso online:https://doi.org/10.3847/1538-4357/ae4bd7
Tags: Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!

Documenti analoghi