Simulations of astrophysical dynamos

Simulations of Buoyant Plumes in Solar Prominences

Simulations of chromospheric heating by ambipolar diffusion

Simulations of magneto-acoustic pulsations in atmospheres of rapidly oscillating Ap stars

Simulations of magneto-hydrodynamic waves in atmospheres of roAp stars

Simulations of Prominence Formation in the Magnetized Solar Corona by Chromospheric Heating

Simulations of stellar convection with CO5BOLD

Simulations of stellar convection, pulsation and semiconvection

Simulations of the IMF in Clusters

Simulations of the Magneto-rotational Instability in Core-Collapse Supernovae

Simulations of the solar near-surface layers with the CO5BOLD, MURaM, and Stagger codes

Simulations of Winds of Weak-Lined T Tauri Stars. II.: The Effects of a Tilted Magnetosphere and Planetary Interactions

Simulations of Winds of Weak-Lined T Tauri Stars: The Magnetic Field Geometry and The Influence of the Wind on Giant Planet Migration

Simultaneous Multi-Wavelength Observations of Magnetic Activity in Ultracool Dwarfs. III. X-ray, Radio, and H-alpha Activity Trends in M and L Dwarfs

Simultaneous Observation of Reconnection Inflow and Outflow Associated with the 2010 August 18 Solar Flare

Simultaneous Observations of the Chromosphere with TRACE and SUMER

Simultaneous solution of Kompaneets equation and Radiative Transfer equation in the photon energy range 1 - 125 KeV

Single peaked CO emission line profiles from the inner regions of protoplanetary disks

Single pulse analysis of PSR B1133+16 at 8.35 GHz and carousel circulation time

Single-degenerate type Ia supernovae without hydrogen contamination