Dynamical SPH + N--body code for chemo--photometric evolution of disk galaxies

Computer Science

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Scientific paper

The chemical and photometric evolution of star forming disk galaxies is investigated. Numerical simulations of the complex gasdynamical flows are based on our own coding of the Chemo -- Dynamical Smoothed Particle Hydrodynamical (CD -- SPH) approach, which incorporates the effects of star formation. As a first application, the model is used to describe the chemical and photometric evolution of a disk galaxy like the Milky Way.

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