This is a summary of the 2013 release of the plasma simulation code Cloudy. Cloudy
models the ionization, chemical, and thermal state of material that may be exposed to an …

Aims. We present and test chemical models for three-dimensional hydrodynamical
simulations of galaxies. We explore the effect of changing key parameters such as …

The previous calculations of the Solar Spectral Irradiance (SSI) by the Solar Radiation
Physical Modeling, version 2 system, are updated in this work by including new molecular …

Photodissociation processes are of great importance for modeling interstellar chemistry
since it is a key destruction pathway for small molecules. Here, we present a detailed ab …

A series of computations based on multichannel quantum defect theory have been
performed in order to produce the cross sections of rotational transitions (excitations N i+ …

Here, we present our current updates to the gas-phase chemical reaction rates and
molecular lines in the spectral synthesis code cloudy, and its implications in spectroscopic …

Studies measuring the chemical abundances of the neutral gas in star-forming galaxies
(SFGs) require ionization correction factors (ICFs) to accurately measure their metal …

The photodissociation process of magnesium oxide (MgO) may be a main source of the
magnesium atom in planetary exospheres due to the impact events on planets. In this work …

Photodissociation by ultraviolet photons is the key destruction pathway for aluminium
monofluoride (AlF) in the envelope of the carbon star IRC+ 10216 from the stellar …

We present results of our numerical simulation of three H2-bearing damped Lyman α
absorbers (DLAs) in the redshift interval∼ 2–3. The systems we have modelled are the …