Computer Science
Scientific paper
Sep 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3...91b&link_type=abstract
Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 91-94
Computer Science
2
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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