3D models for self-gravitating, rotating magnetic interstellar clouds

3D models of radiatively driven colliding winds in massive O+O star binaries - II. Thermal radio to sub-mm emission

3D models of radiatively driven colliding winds in massive O+O star binaries - III. Thermal X-ray emission

3D molecular line formation in dwarf carbon-enhanced metal-poor stars

3D non-LTE line formation in the solar photosphere and the solar oxygen abundance

3D non-LTE spectrum synthesis for Type Ia supernovae

3D Null Point Reconnection Regimes

3D numerical cosmological radiative transfer in an inhomogeneous medium

3D Numerical Experimentation on the Core Helium Flash of low-mass Red Giants

3D numerical MHD modeling of sunspots with radiation transport

3D numerical model of the Omega Nebula (M17): simulated thermal X-ray emission

3D numerical models of magnetic field evolution in galaxies interacting with the ICM

3d Numerical Models of the Chromosphere, Transition Region, and Corona

3D Numerical Relativity at NCSA

3D numerical relativity using collisionless particles: gauge conditions

3D Numerical Simulation and Stereoscopic Observations of Coronal Jets

3D numerical simulation of gaseous flows structure in semidetached binaries

3D Numerical Simulations of AGN Outflows in Clusters and Groups

3D Numerical Simulations of f-Mode Propagation Through Magnetic Flux Tubes

3D numerical simulations of magnetic field evolution in barred galaxies and in spiral galaxies under influence of tidal forces