Chemo - Photometric evolution of star forming disk galaxy
| dc.creator | Berczik, Peter | |
| dc.date | 2000-01-06 | |
| dc.date.accessioned | 2026-07-07T01:51:35Z | |
| dc.date.available | 2026-07-07T01:51:35Z | |
| dc.description | 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. | |
| dc.description | 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) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0001093 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0001093 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/340 | |
| dc.subject | Astrophysics | |
| dc.title | Chemo - Photometric evolution of star forming disk galaxy | |
| dc.type | text |