Ultraviolet Radiation Fields in Star-forming Disk Galaxies: Numerical Simulations with TIGRESS-NCR

With numerical simulations that employ adaptive ray-tracing (ART) for radiative transfer at the same time as evolving gas magnetohydrodynamics, thermodynamics, and photochemistry, it is possible to obtain a high-resolution view of ultraviolet (UV) fields and their effects in realistic models of the...

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Veröffentlicht in:	The Astrophysical journal 2024-11, Vol.975 (2), p.173
Hauptverfasser:	Linzer, Nora B., Kim, Jeong-Gyu, Kim, Chang-Goo, Ostriker, Eve C.
Format:	Artikel
Sprache:	eng
Schlagworte:	Aromatic hydrocarbons Astronomical models Cosmic dust Density Disk galaxies Dust emission Emission Emission measurements Galaxy distribution High resolution Interstellar gas Interstellar matter Interstellar medium Interstellar radiation field Ionization Ionizing radiation Magnetohydrodynamical simulations Magnetohydrodynamics Mathematical analysis Numerical simulations Photochemistry Photoelectricity Photoionization Polycyclic aromatic hydrocarbons Radiation Radiative transfer Ray tracing Simulation Solar neighborhood Spatial distribution Star formation Thermodynamics Ultraviolet radiation Wavelengths
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