231 citations · 474 across the 8 of their papers we have counts for
8 papers
Turbulence and Vorticity in Galaxy Clusters Generated by Structure Formation
F. Vazza, T. W. Jones, M. Brüggen +4
Turbulence is a key ingredient for the evolution of the intracluster medium, whose properties can be predicted with high resolution numerical simulations. We present initial result…
Vorticity, Shocks and Magnetic Fields in Subsonic, ICM-like Turbulence
David H. Porter, T. W. Jones, Dongsu Ryu
We analyze high resolution simulations of compressible, MHD turbulence with properties resembling conditions in galaxy clusters. The flow is driven to turbulence Mach number $\math…
MHD Turbulence Simulation in a Cosmic Structure Context
T. W. Jones, D. H. Porter, D. Ryu +1
The gaseous media of galaxy clusters and cosmic filaments, which constitute most of the baryonic matter in the universe, is highly dynamic. It is also probably turbulent, although…
Cluster Turbulence: Simulation Insights
T. W. Jones, David H. Porter, Dongsu Ryu +1
Cluster media are dynamical, not static; observational evidence suggests they are turbulent. High-resolution simulations of the intracluster media (ICMs) and of idealized, similar…
Convective-reactive proton-C12 combustion in Sakurai's object (V4334 Sagittarii) and implications for the evolution and yields from the first generations of stars
Falk Herwig, Marco Pignatari, Paul R. Woodward +5
Depending on mass and metallicity as well as evolutionary phase, stars occasionally experience convective-reactive nucleosynthesis episodes. We specifically investigate the situati…
The Hydrodynamic Environment for the s Process in the He-Shell Flash of AGB Stars
Paul R. Woodward, David H. Porter, Falk Herwig +3
The He-shell flash convection in AGB stars is the site for the high-temperature component of the s-process in low- and intermediate mass giants, driven by the Ne22 neutron source.…