DISRUPTION OF DWARF SATELLITE GALAXIES WITHOUT DARK MATTER
The evolution of a satellite galaxy of a Milky Way like galaxy has been studied using N-Body simulations. The initial satellites, containing 106 particles, have been simulated by a Plummer sphere, while the potential of the host galaxy is a three component rigid potential: disc, bulge and dark matte...
में बचाया:
| में प्रकाशित: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| मुख्य लेखकों: | , |
| स्वरूप: | Artigo |
| भाषा: | Inglês |
| प्रकाशित: |
Universidad Nacional Autónoma de México
2011
|
| विषय: | |
| ऑनलाइन पहुंच: | https://www.redalyc.org/articulo.oa?id=57121297017 |
| टैग: |
कोई टैग नहीं, इस रिकॉर्ड को टैग करने वाले पहले व्यक्ति बनें!
|