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,...
Na minha lista:
| Publicado no: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Principais autores: | , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Universidad Nacional Autónoma de México
2011
|
| Assuntos: | |
| Acesso em linha: | https://www.redalyc.org/articulo.oa?id=57121297021 |
| Tags: |
Sem tags, seja o primeiro a adicionar uma tag!
|