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- (abs, pdf) Lee et al., How Do Star-Forming Galaxies at Z>3 Assemble Their Masses?
- (abs, pdf) Hopkins et al., Why Are AGN and Host Galaxies Misaligned?
- (abs, pdf) Tremblin et al., 3D simulations of pillars formation around HII regions: the importance of shock curvature
- (abs, pdf) Stacy et al., Effect … Continue Reading ››
- (abs, pdf) Bournaud et al., An Observed Link between Active Galactic Nuclei and Violent Disk Instabilities in High-Redshift Galaxies
- (abs, pdf) Salucci et al., Dwarf spheroidal galaxy kinematics and spiral galaxy scaling laws
- (abs, pdf) Tonnesen & Cen, Effects on Galaxy Evolution: Pair Interactions versus Environment
- (abs, pdf) Khandai et al., The Formation of Galaxies Hosting z~6 Quasars
- (abs, pdf) Cen, Inconsequence of Galaxy Major Mergers in Driving Star Formation at z>1: Insights from Cosmological Simulations
- (abs, pdf) Silvia et al., Numerical Simulations of Supernova Dust Destruction. II. Metal-Enriched Ejecta Knots
- (abs, pdf) Danovich et al., Co-planar streams, pancakes, and angular-momentum exchange in high-z disc galaxies
- (abs, pdf) Cen, Far-Infrared Properties of Lyman Break Galaxies from Cosmological Simulations
- (abs, pdf) Tissera et al., Chemical signatures of formation processes in the stellar populations of simulated galaxies
- (abs, pdf) Kirby et al., Metals Removed by Outflows from Milky Way Dwarf Spheroidal Galaxies
Larne Pekowsky (CRA)
- CUDA FFT is a drop-in replacement for FFTW. Because of the memory bandwidth, CUDA is faster above 2^14 element FFTs in 1D. Tested on GTX 580.
- Used in LIGO data analysis.
- (abs, pdf) Haworth & Harries, Radiation hydrodynamics of triggered star formation: the effect of the diffuse radiation field
- (abs, pdf) Park & Ricotti, Accretion onto Black Holes from Large Scales Regulated by Radiative Feedback. II. Growth Rate and Duty Cycle
- (abs, pdf) Hopkins et al., Stellar Feedback in Galaxies and the Origin of Galaxy-scale Winds
Simulating the Universe