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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 effect 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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Keywords: Galaxy evolution; Milky way; SPH; Star formation in SPH

Document Type: Research Article

Affiliations: Main Astronomical Observatory, Ukrainian National Academy of Sciences, UA-03680, Golosiiv, Kiev-121, Ukraine

Publication date: 01 January 2002

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