New NIR diagnostic diagrams using [C I]/Paγ and H2 1-0 O(5)/PAH 3.3μm ratios correlate with radiation field hardness and distinguish star formation, AGN, and shock excitation in galaxy nuclei.
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High CR ionization rates (above 10^-13 s^-1) in AGN and starburst models produce enhanced low-ionization emission that matches observations without super-solar metallicities and suggests revised BPT diagram boundaries.
RTGen applies post-processing Monte Carlo radiative transfer to six hydrodynamic galaxy simulations to compute dust temperatures, SEDs, continuum images, and molecular line emission while testing the effects of dust modeling choices.
citing papers explorer
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Near-infrared diagnostic diagrams of the gas ionization sources in nearby galaxies: a JWST NIRSpec view
New NIR diagnostic diagrams using [C I]/Paγ and H2 1-0 O(5)/PAH 3.3μm ratios correlate with radiation field hardness and distinguish star formation, AGN, and shock excitation in galaxy nuclei.
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Cosmic Ray Ionization of Low-Excitation Lines in Active Galactic Nuclei and Starburst Galaxies
High CR ionization rates (above 10^-13 s^-1) in AGN and starburst models produce enhanced low-ionization emission that matches observations without super-solar metallicities and suggests revised BPT diagram boundaries.
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Dust and gas modelling in radiative transfer simulations of disc-dominated galaxies with RADMC-3D
RTGen applies post-processing Monte Carlo radiative transfer to six hydrodynamic galaxy simulations to compute dust temperatures, SEDs, continuum images, and molecular line emission while testing the effects of dust modeling choices.
- Impact of Primordial Black Hole population on 21 cm observables at high redshift