The 2013 Release of Cloudy
arXiv:1302.4485
Abstract
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 external radiation field or other source of heating, and predicts observables such as emission and absorption spectra. It works in terms of elementary processes, so is not limited to any particular temperature or density regime. This paper summarizes advances made since the last major review in 1998. Much of the recent development has emphasized dusty molecular environments, improvements to the ionization / chemistry solvers, and how atomic and molecular data are used. We present two types of simulations to demonstrate the capability of the code. We consider a molecular cloud irradiated by an X-ray source such as an Active Nucleus and show how treating EUV recombination lines and the full SED affects the observed spectrum. A second example illustrates the very wide range of particle and radiation density that can be considered.
Major review article to be published in RevMexAA. 27 pages, 18 figures
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- Spectroscopic modelling of four neutron star low-mass X-ray binaries using CLOUDY
- Physical conditions in highz optically thin C III absorbers: Origin of cloud sizes and associated correlations
- Analogs of primeval galaxies two billion years after the Big Bang
- Physical conditions and redshift evolution of optically thin C III absorbers: Low-z sample
- Metals and a Search for Molecules in the Distant Universe: Magellan MIKE Observations of sub-DLAs at 2<z<3
- Spectroscopic modelling of two high-mass X-ray binaries, Cyg X--3 and 4U 1538--522
- Absorption systems at as a probe of the circum galactic medium: a probabilistic approach
- The highly obscured Seyfert 2 nucleus in NGC 1448 observed with MUSE
- Quasars: from the Physics of Line Formation to Cosmology
- Are Boltzmann Plots of Hydrogen Balmer lines a tool for identifying a subclass of S1 AGN?