Simulations of stars and gas in spiral galaxies

<p>A new code, DUAL, is developed to model the 2D dynamics of stars and gas in spiral galaxies. DUAL combines grid-based hydrodynamics and N-body techniques.</p> <p>A triaxial model of the bulge of M31 is constructed from its surface brightness profile and shown, using hydrodynamic...

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Bibliographic Details
Main Author: Berman, S
Format: Thesis
Published: 2002