We review the use of emission lines for understanding galaxy evolution, focusing on
excitation source, metallicity, ionization parameter, ISM pressure, and electron density. We …

Radiation transport plays a crucial role in star formation models, as certain questions within
this field cannot be accurately addressed without taking it into account. Given the high …

Hydrogen emission lines can provide extensive information about star-forming galaxies in
both the local and high-redshift Universe. We present a detailed Lyman continuum (LyC) …

Photoionization models frequently assume constant temperature or density within H ii
regions. We investigate this assumption by measuring the detailed temperature and density …

Context. To understand the structures of complex astrophysical objects, 3D numerical
simulations of radiative transfer processes are invaluable. For Monte Carlo radiative transfer …

We present an efficient heating/cooling method coupled with chemistry and UV radiative
transfer that can be applied to numerical simulations of the interstellar medium (ISM). We …

Abstract The Messenger Interface Monte Carlo Mappings V (M 3) is a photoionization code
adopting the fully self-consistent Monte Carlo radiative transfer (MCRT) technique, which …

We present arepo-mcrt, a novel Monte Carlo radiative transfer radiation-hydrodynamics
(RHD) solver for the unstructured moving-mesh code arepo. Our method is designed for …

We report on a new capability added to our general relativistic radiation-
magnetohydrodynamics code, Cosmos++: an implicit Monte Carlo (IMC) treatment for …

We present a new smoothed particle hydrodynamics-radiative transfer method (sph-m1rt)
that is coupled dynamically with sph. We implement it in the (task-based parallel) swift …