ORIGIN AND EVOLUTION OF THE SAGITTARIUS DWARF GALAXY USING N-BODY SIMULATIONS
We study the evolution of the Sagittarius dwarf galaxy by means of N-body numerical simulations. We find the initial conditions of the orbit of the satellite, such that after a time shorter than 10 Gyrs, this astrophysical object has the position and galactocentric radial velocity currently observed...
Furkejuvvon:
| Publikašuvnnas: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Váldodahkkit: | , |
| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
Universidad Nacional Autónoma de México
2011
|
| Fáttát: | |
| Liŋkkat: | https://www.redalyc.org/articulo.oa?id=57121297027 |
| Fáddágilkorat: |
Eai fáddágilkorat, Lasit vuosttaš fáddágilkora!
|