activity
19952008
most citedThe RAGE radiation-hydrodynamic code

382 citations · 968 across the 12 of their papers we have counts for

collaborators

12 papers

physics.comp-ph2008★ 382 cited

The RAGE radiation-hydrodynamic code

Michael Gittings, Robert Weaver, Michael Clover +9

We describe RAGE, the ``Radiation Adaptive Grid Eulerian'' radiation-hydrodynamics code, including its data structures, its parallelization strategy and performance, its hydrodynam…

astro-ph2008★ 69 cited

The Origin and Kinematics of Cold Gas in Galactic Winds: Insight from Numerical Simulations

Akimi Fujita, Crystal L. Martin, Mordecai-Mark Mac Low +2

We study the origin of Na I absorbing gas in ultraluminous infrared galaxies motivated by the recent observations by Martin of extremely superthermal linewidths in this cool gas. W…

gr-qc2002★ 133 cited

Gravitational Waves from Gravitational Collapse

Kimberly C. B. New

Gravitational wave emission from the gravitational collapse of massive stars has been studied for more than three decades. Current state of the art numerical investigations of coll…

gr-qc2001

Rotational Instabilities and Centrifugal Hangup

Kimberly C. B. New, Joan M. Centrella

One interesting class of gravitational radiation sources includes rapidly rotating astrophysical objects that encounter dynamical instabilities. We have carried out a set of simula…

astro-ph2000★ 149 cited

Dynamical Rotational Instability at Low

Joan M. Centrella, Kimberly C. B. New, Lisa L. Lowe +1

Dynamical instability is shown to occur in differentially rotating polytropes with N = 3.33 and . This instability has a strong m=1 mode, although the m=2, 3, a…

astro-ph2000★ 38 cited

Evolution of Differentially Rotating Supermassive Stars to the Onset of Bar Instability

Kimberly C. B. New, Stuart L. Shapiro

Thermal emission from a rotating, supermassive star will cause the configuration to contract slowly and spin up. If internal viscosity and magnetic fields are sufficiently weak, th…