activity
20062009
most citedThe effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas

956 citations · 1.3k across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2009

First Light Sources at the End of the Dark Ages: Direct Observations of Population III Stars, Proto-Galaxies, and Supernovae During the Reionization Epoch

Jeff Cooke, Asantha Cooray, Ranga-Ram Chary +16

The cosmic dark ages are the mysterious epoch during which the pristine gas began to condense and ultimately form the first stars. Although these beginnings have long been a topic…

astro-ph2008956 cited

The effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas

Robert P. C. Wiersma, Joop Schaye, Britton D. Smith

Radiative cooling is central to a wide range of astrophysical problems. Despite its importance, cooling rates are generally computed using very restrictive assumptions, such as col…

astro-ph200778 cited

Modeling of Emission Signatures of Massive Black Hole Binaries: I Methods

Tamara Bogdanovic, Britton D. Smith, Steinn Sigurdsson +1

We model the electromagnetic signatures of massive black hole binaries (MBHBs) with an associated gas component. The method comprises numerical simulations of relativistic binaries…

astro-ph2007136 cited

Metal Cooling in Simulations of Cosmic Structure Formation

Britton D. Smith, Steinn Sigurdsson, Tom Abel

The addition of metals to any gas can significantly alter its evolution by increasing the rate of radiative cooling. In star-forming environments, enhanced cooling can potentially…

astro-ph200781 cited

The Transition from the First Stars to the Second Stars in the Early Universe

Britton D. Smith, Steinn Sigurdsson

We observe a sharp transition from a singular, high-mass mode of star formation, to a low-mass dominated mode, in numerical simulations, at a metallicity of 10^-3 Zsolar. We incorp…

astro-ph2006

Electromagnetic Signatures of Massive Black Hole Binaries

Tamara Bogdanovic, Britton D. Smith, Michael Eracleous +1

We model the electromagnetic emission signatures of massive black hole binaries (MBHBs) with an associated gas component. The method comprises numerical simulations of relativistic…