2000/01/06 by Peter Berczik, Berczik, Peter
Engineering · Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Fluid Dynamics Simulations and Interactions #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0001093
4 pages, LaTeX2e, using the eslab.cls file, presented as a poster in the 33rd ESLAB Symp. "Star formation from the small to the large scale", Noordwijk, The Netherlands, 2-5 November 1999, (F. Favata, A.A. Kaas & A. Wilson eds, ESA SP-445, 2000)
arxiv created 2000/01/06 · arxiv updated 2009/12/01
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.