Publications
Years
- Three-dimensional Simulations of Magnetized Superbubbles: New Insights into the Importance of MHD Effects on Observed Quantities (2009)
- The role of jets in the formation of planets, stars and galaxies (2009)
- Large-scale 3D Simulations of Protostellar Jets: Long-term Stability and Jet Rotation (2009)
- Large-Scale 3D Simulations of Protostellar Jets (2009)
- The Possibly Remnant Massive Outflow in G5.89-0.39. I. Observations and Initial Magnetohydrodynamic Simulations (2006)
- Controlling the collimation and rotation of hydromagnetic disc winds (2006)
- GRMHD Simulations of Disk/Jet Systems: Application to the Inner Engines of Collapsars (2005)
- JETGET - An analysis and visualization tool for (magneto-)hydrodynamic jet simulations (2004)
- Three-dimensional Simulations of Jets from Keplerian Disks: Self-regulatory Stability (2003)
- Three-Dimensional Simulations of Jets from Keplerian Disks: Stability Issues (2003)
- The First Niels Bohr Summer Institute: Beaming and Jets in Gamma Ray Bursts (2002)
- Initial magnetic field configurations for 3-dimensional simulations of astrophysical jets (2001)
- Numerical simulations of astrophysical jets from Keplerian discs - III. The effects of mass loading (1999)
- Numerical simulations of protostellar jets with multi-pressure components from Keplerian disks. (1999)
- Jets in Protostellar Systems (1999)
- Numerical Simulations of Astrophysical Jets from Keplerian Disks. II. Episodic Outflows (1997)
- Numerical Simulations of Astrophysical Jets from Keplerian Disks. I. Stationary Models (1997)
- Episodic jets from black holes and protostars (1997)
- Forbidden-Line Formation in Hydromagnetic Disk Winds. II. Line Profiles (1994)
- Forbidden Line Formation in Hydromagnetic Disk Winds. I. Oblique Shocks (1993)
Multimedia
Animation of increasing Z slices from the bow-shock inwards. Simulated flying into the jet. Visualization done by SHAPE.
BP animation of slit movement accross jet for SII. Images are LOG scale. Visualization done by SHAPE.
BP color animation. H = Blue, OII = Orange, FeII = Red. The jet is inclined at x=30 deg, y = 30 deg. All images are in a LOG scale. Visualization done by SHAPE.
PP color animation. H = Blue, OII = Orange, FeII = Red. The jet is inclined at x=30 deg, y = 30 deg. All images are in a LOG scale. Visualization done by SHAPE.
MU color animation. H = Blue, OII = Orange, FeII = Red. The jet is inclined at x=30 deg, y = 30 deg. All images are in a LOG scale. Visualization done by SHAPE.
PP FeII animation. First sequence is grey-scale, second is temperature, third is z-velocity. No inclination. Visualization done by SHAPE.
MU color animation. H = Blue, OII = Orange, FeII = Red. The jet is inclined at x=30 deg, y = 30 deg. All images are in a LOG scale. Visualization done by SHAPE.
MU SII animation. First sequence is grey-scale, second is temperature, third is z-velocity. The jet is inclined at x=30 deg, y = 30 deg. Visualization done by SHAPE.
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Contact Us
Questions, comments or inquiries about MHD
Contact Details
- Rachid Ouyed
[email protected] - +1 (403) 210-8418
- Quark Nova Project
Department of Physics and Astronomy
University of Calgary, Calgary, Alberta, Canada