activity
19962011
most citedTurbulence and Magnetic Fields in the Large Scale Structure of the Universe

432 citations · 815 across the 14 of their papers we have counts for

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Showing 2005 · astro-phShow all

7 papers · 2 filters

astro-ph2005

The 21 Centimeter Background from the Cosmic Dark Ages: Minihalos and the Intergalactic Medium before Reionization

Paul R. Shapiro, Kyungjin Ahn, Marcelo A. Alvarez +3

The H atoms inside minihalos (i.e. halos with virial temperatures T_vir < 10^4 K, in the mass range roughly from 10^4 M_sun to 10^8 M_sun) during the cosmic dark ages in a LambdaCD…

astro-ph2005

The 21-cm Background from the Cosmic Dark Ages: Minihalos and the Intergalactic Medium before Reionization

Kyungjin Ahn, Paul R. Shapiro, Marcelo A. Alvarez +3

The H atoms inside minihalos (i.e. halos with virial temperatures T_vir < 10^4 K, in the mass range roughly from 10^4 M_sun to 10^8 M_sun) during the cosmic dark ages in a LCDM uni…

astro-ph2005

Molecular cloud evolution. I. Molecular cloud and thin CNM sheet formation

Enrique Vazquez-Semadeni, Dongsu Ryu, Thierry Passot +2

We discuss molecular cloud formation by large-scale supersonic compressions in the diffuse warm neutral medium (WNM). Initially, a shocked layer forms, and within it, a thin cold l…

astro-ph2005

3D Simulations of MHD Jet Propagation Through Uniform and Stratified External Environments

S. M. O'Neill, I. L. Tregillis, T. W. Jones +1

We present a set of high-resolution 3D MHD simulations of steady light, supersonic jets, exploring the influence of jet Mach number and the ambient medium on jet propagation and en…

astro-ph2005

Density Power Spectrum of Compressible Hydrodynamic Turbulent Flows

Jongsoo Kim, Dongsu Ryu

Turbulent flows are ubiquitous in astrophysical environments, and understanding density structures and their statistics in turbulent media is of great importance in astrophysics. I…

astro-ph2005

Numerical Relativistic Hydrodynamics Based on the Total Variation Diminishing Scheme

Eunwoo Choi, Dongsu Ryu

This paper describes a multidimensional hydrodynamic code which can be used for studies of relativistic astrophysical flows. The code solves the special relativistic hydrodynamic e…