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,...
Kaydedildi:
| Yayımlandı: | Revista Mexicana de Astronomía y Astrofísica |
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| Asıl Yazarlar: | , , |
| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
Universidad Nacional Autónoma de México
2011
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| Konular: | |
| Online Erişim: | https://www.redalyc.org/articulo.oa?id=57121297021 |
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