activity
20052024
most citedThe 2013 Release of Cloudy

446 citations · 2k across the 32 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

6 papers · 1 filter

astro-ph.CO2013★ 146 cited

The primordial helium abundance from updated emissivities

Erik Aver, Keith A. Olive, R. L. Porter +1

Observations of metal-poor extragalactic H II regions allow the determination of the primordial helium abundance, Y_p. The He I emissivities are the foundation of the model of the…

astro-ph.CO2013★ 12 cited

Expanded Iron UTA spectra -- probing the thermal stability limits in AGN clouds

G. J. Ferland, R. Kisielius, F. P. Keenan +5

The Fe unresolved transition array (UTAs) produce prominent features in the 15-17?A wavelength range in the spectra of Active Galactic Nuclei (AGN). Here we present new calculation…

astro-ph.CO2012★ 11 cited

Hydrogen Two-Photon Continuum Emission from the Horseshoe Filament in NGC 1275

R. M. Johnstone, R. E. A. Canning, A. C. Fabian +5

Far ultraviolet emission has been detected from a knot of Halpha emission in the Horseshoe filament, far out in the NGC 1275 nebula. The flux detected relative to the brightness of…

astro-ph.CO2012★ 109 cited

Improved He I Emissivities in the Case B Approximation

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

We update our prior work on the case B collisional-recombination spectrum of He I to incorporate \textit{ab initio} photoionisation cross-sections. This large set of accurate, self…

astro-ph.CO2010★ 12 cited

Broad and Luminous [OIII] and [NII] in Globular Cluster ULXs

Ryan L. Porter

We consider an accretion-disc origin for the broad and luminous forbidden-line emission observed in ultraluminous X-ray (ULX) sources CXOJ033831.8-352604 and XMMU 122939.7+075333 i…

astro-ph.CO2009★ 92 cited

Implications of infalling Fe II - emitting clouds in active galactic nuclei: anisotropic properties

Gary J. Ferland, Chen Hu, Jian-Min Wang +4

We investigate consequences of the discovery that Fe II emission in quasars, one of the spectroscopic signatures of "Eigenvector 1", may originate in infalling clouds. Eigenvector…