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,...
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| Gepubliceerd in: | Revista Mexicana de Astronomía y Astrofísica |
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| Hoofdauteurs: | , , |
| Formaat: | Artigo |
| Taal: | Inglês |
| Gepubliceerd in: |
Universidad Nacional Autónoma de México
2011
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| Onderwerpen: | |
| Online toegang: | https://www.redalyc.org/articulo.oa?id=57121297021 |
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