SUPERNOVA FEEDBACK AND THE BEND OF THE TULLY-FISHER RELATION
We have studied the origin of the Tully-Fisher relation by analysing hydrodynamical simulations in a ACDM universe. We found that smaller galaxies exhibit lower stellar masses than those predicted by the linear fit to high mass galaxies (fast rotators), consistently with observations. In this model,...
Guardado en:
| Publicado en: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Autores principales: | , , |
| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
Universidad Nacional Autónoma de México
2011
|
| Materias: | |
| Acceso en línea: | https://www.redalyc.org/articulo.oa?id=57121297021 |
| Etiquetas: |
Sin Etiquetas, Sea el primero en etiquetar este registro!
|