3-D Monte Carlo radiative transfer calculation of resonance line formation in the inhomogeneous expanding stellar wind

3-D Photoionization Structure and Distances of Planetary Nebulae IV. NGC 40

3-D radiative transfer in clumped hot star winds I. Influence of clumping on the resonance line formation

3-D Radiative Transfer Modeling of Structured Winds in Massive Hot Stars with Wind3D

325 MHz VLA Observations of Ultracool Dwarfs TVLM 513-46546 and 2MASS J0036+1821104

3D Coronal Slow Modes: Towards 3D Seismology

3D evolution of a filament disappearance event observed by STEREO

3D hydrodynamical CO5BOLD model atmospheres of late-type giants: chemical abundances from molecular lines

3D hydrodynamical model atmospheres: a tool to correct radial velocities and parallaxes for Gaia

3D hydrodynamical simulations of a proton ingestion episode in a low-metallicity asymptotic giant branch star

3D hydrodynamical simulations of stellar photospheres with the CO5BOLD code: photometric colors of a late-type giant

3D LTE spectral line formation with scattering in red giant stars

3D MHD Flux Emergence Experiments: Idealized models and coronal interactions

3D MHD model of the collapse and fragmentation of turbulent prestellar core

3D MHD Simulations of Disk Accretion onto Magnetized Stars: Numerical Approach and Sample Simulations

3D MHD simulations of subsurface convection in OB stars

3D Model Atmospheres of Red Giant Stars

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