COMPLEX MODELING THE CHEMO-PHOTOMETRIC EVOLUTION OF DISK GALAXY

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Abstract:

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.

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

Document Type: Research Article

DOI: http://dx.doi.org/10.1080/10556790215589

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

Publication date: January 1, 2002

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