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Sub-mm observations of protoplanetary disks now approach the acuity needed to measure the turbulent broadening of molecular lines. These measurements constrain disk angular momentum transport, and fur...
In previous studies, we examined turbulence-flame interactions in carbon-burning thermonuclear flames in Type Ia supernovae. In this study, we consider turbulence-flame interactions in the trailing ox...
In the presence of large-scale vortical motions and/or magnetic-field strains, the turbulent cross helicity (velocity--magnetic-field correlation in fluctuations) may contribute to the turbulent elect...
Direct numerical simulations of the interaction of a premixed flame with driven, subsonic, homogeneous, isotropic,Kolmogorov-type turbulence in an unconfined system are used to study the mechanisms de...
We present high-resolution computer simulations of dust dynamics and planetesimal formation in turbulence generated by the magnetorotational instability. We show that the turbulent viscosity associate...
We study the properties of chaotic motions in the intra cluster medium using a set of 20 galaxy clusters simulated with large dynamical range, using the Adaptive Mesh Refinement code ENZO (e.g. Norman...
We characterize the infall rate onto protostellar systems forming in self-gravitating radiation-hydrodynamic simulations. Using two dimensionless parameters to determine disks' susceptability to gravi...
We performed a numerical experiment designed for core formation in a self-gravitating, magnetically supercritical, supersonically turbulent, isothermal cloud. A density probability distribution functi...
Theoretical modeling of the driving processes of solar-like oscillations is a powerful way of understanding the properties of the convective zones of solar-type stars. In this framework, the descripti...
Resolution Issues in the Collapse and Fragmentation of Turbulent Molecular Cloud Cores。
A Model for the Cross Section of a Turbulent, Radiative Jetor Wake。
Recent Advances in the Collapse and Fragmentation of Turbulent Molecular Cloud Cores。
An Optical Spectroscopic Study of HH 110:a Turbulent Mixing Layer?
[WC] Stellar wind turbulent outflows feeding the ism。
We describe ZEUS-MP: a Multi-Physics, Massively-Parallel, Message-Passingcode for astrophysical .uid dynamics simulations in 3 dimensions. ZEUS-MP is afollow-on to the sequential ZEUS-2D and ZEUS-3D c...

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