COMPLEX MODELING THE CHEMO-PHOTOMETRIC EVOLUTION OF DISK GALAXY
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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Document Type: Research Article
Affiliations: Main Astronomical Observatory, Ukrainian National Academy of Sciences, UA-03680, Golosiiv, Kiev-121, Ukraine
Publication date: 01 January 2002