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Williams, P. R. |
Volume |
Paper Title |
Page Number |
Authors |
126 |
A New Numerical Method For Solving Partial Differential Equations - Selected Lagrangian Weights |
571 |
Williams, P. R.; Nelson, A. H. |
126 |
The Formation of Disk Galaxies Using TREESPH on a Parallel Computer |
573 |
Williams, P. R.; Nelson, A. H. |
182 |
Numerical Simulation of the Formation of an SBC Disk Galaxy |
549 |
Williams, P. R.; Nelson, A. H. |
182 |
The Relationship Between the Initial Conditions and Morphology of Spiral Galaxies: Numerical Simulations |
551 |
Williams, P. R.; Nelson, A. H. |
245 |
Time Scales and the Formation of Low Surface Brightness Galaxies |
460 |
Williams, P. R.; Nelson, A. H. |
245 |
Potogalaxies and the Hubble Sequence |
463 |
Williams, P. R.; Nelson, A. H. |
275 |
The Role of Proto--Dwarf Galaxies in the Formation of Galaxy Disk |
413 |
Williams, P. R.; Nelson, A. H. |
275 |
Proto--Galaxies and the Hubble Sequence |
414 |
Williams, P. R.; Nelson, A. H. |
275 |
The Dangers of Constraining the Kernel Radius in SPH Galaxy Simulations |
452 |
Williams, P. R.; Churches, D. K.; Nelson, A. H. |
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