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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. | 
		 
			
			| 540 | 
			Dynamical Modeling of the Broad Line Region of NGC 4151 | 
			9 | 
			Ramachandran, M.; Robinson, J. H.; Bentz, M. C.; Williams, P. R.; Treu, T.; De Rosa, G. | 
		 
	 
					 
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