This paper describes the most important differences between Cloudy 90 and Cloudy 94, the most recent upgrade of the code which has now been posted on the WWW. It also describes the upgrade of the grain model in Cloudy which is currently underway
Aims. We present a comparison between independent computer codes, modeling the physics and chemistr...
This is the final version of the article. Available from OUP via the DOI in this record.The dataset ...
We study the effect of stellar feedback (photodissociation/ionization, radiation pressure, and winds...
We describe the 2017 release of the spectral synthesis code Cloudy , summa- rizing the many improvem...
This is a summary of the 2013 release of the plasma simulation code CLOUDY. CLOUDY models the ioniza...
We describe the 2017 release of the spectral synthesis code Cloudy, summarizing the many improvement...
We describe the 2017 release of the spectral synthesis code Cloudy, summarizing the many improvement...
We describe a new atomic and molecular database we developed for use in the spectral synthesis code ...
A large-scale code called Cloudy was designed to simulate non-equilibrium plasmas and predict their ...
Here we present our current updates of the gas-phase chemical reaction rates and molecular lines in ...
We developed a new quick pseudo-3D photoionization code based on Cloudy (G. Ferland) and IDL (RSI) t...
Ever since the pioneering study of Spitzer, it has been widely recognized that grains play an import...
This is the final version of the article. Available from Oxford University Press via the DOI in this...
Recent improvements to the plasma simulation code Cloudy will allow the inclusion of model ions and...
A three-dimensional smoothed particle hydrodynamics model has been extended to study the radiation-d...
Aims. We present a comparison between independent computer codes, modeling the physics and chemistr...
This is the final version of the article. Available from OUP via the DOI in this record.The dataset ...
We study the effect of stellar feedback (photodissociation/ionization, radiation pressure, and winds...
We describe the 2017 release of the spectral synthesis code Cloudy , summa- rizing the many improvem...
This is a summary of the 2013 release of the plasma simulation code CLOUDY. CLOUDY models the ioniza...
We describe the 2017 release of the spectral synthesis code Cloudy, summarizing the many improvement...
We describe the 2017 release of the spectral synthesis code Cloudy, summarizing the many improvement...
We describe a new atomic and molecular database we developed for use in the spectral synthesis code ...
A large-scale code called Cloudy was designed to simulate non-equilibrium plasmas and predict their ...
Here we present our current updates of the gas-phase chemical reaction rates and molecular lines in ...
We developed a new quick pseudo-3D photoionization code based on Cloudy (G. Ferland) and IDL (RSI) t...
Ever since the pioneering study of Spitzer, it has been widely recognized that grains play an import...
This is the final version of the article. Available from Oxford University Press via the DOI in this...
Recent improvements to the plasma simulation code Cloudy will allow the inclusion of model ions and...
A three-dimensional smoothed particle hydrodynamics model has been extended to study the radiation-d...
Aims. We present a comparison between independent computer codes, modeling the physics and chemistr...
This is the final version of the article. Available from OUP via the DOI in this record.The dataset ...
We study the effect of stellar feedback (photodissociation/ionization, radiation pressure, and winds...