activity
19982023
most citedThe 2013 Release of Cloudy

446 citations · 1.9k across the 76 of their papers we have counts for

collaborators
Showing 2005 · astro-phShow all

8 papers · 2 filters

astro-ph2005

Physical Conditoins in Orion's Veil II: A Multi-Component Study of the Line of Sight Toward the Trapezium

N. P. Abel, G. J. Ferland, C. R. O'Dell +2

Orion's Veil is an absorbing screen that lies along the line of sight to the Orion H II region. It consists of two or more layers of gas that must lie within a few parsecs of the T…

astro-ph2005

Physical conditions in the ISM towards HD185418

Gargi Shaw, G. J. Ferland, R. Srianand +1

We have developed a complete model of the hydrogen molecule as part of the spectral simulation code Cloudy. Our goal is to apply this to spectra of high-redshift star-forming regio…

astro-ph2005

Molecular hydrogen in the diffuse interstellar medium at high redshift

Raghunathan Srianand, Gargi Shaw, Gary Ferland +2

Physical conditions within DLAs can reveal the star formation history, determine the chemical composition of the associated ISM, and hence document the first steps in the formation…

astro-ph2005

The VLT-UVES survey for molecular hydrogen in high-redshift damped Lyman-alpha systems: Physical conditions in the neutral gas

Raghunathan Srianand, Patrick Petitjean, Cedric Ledoux +2

We study the physical conditions in DLAs, using a sample of 33 systems toward 26 QSOs acquired for a recently completed survey of H_2 by Ledoux et al. (2003). We use the column den…

astro-ph2005

Physical conditions in the Homunculus

Gary J. Ferland, Nick Abel, Kris Davidson +1

Conditions within the Homunculus nebula around Eta Car are determined by many of the same physical processes that occur in molecular clouds in the interstellar medium. But there is…

astro-ph2005

Theoretical He I Emissivities in the Case B Approximation

R. L. Porter, R. P. Bauman, G. J. Ferland +1

We calculate the He I case B recombination cascade spectrum using improved radiative and collisional data. We present new emissivities over a range of electron temperatures and den…