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.
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A review summarizing observations of star formation and gas relations from molecular clouds to entire galaxies, with updated rate calculation prescriptions.
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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.
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Star Formation in the Milky Way and Nearby Galaxies
A review summarizing observations of star formation and gas relations from molecular clouds to entire galaxies, with updated rate calculation prescriptions.