A VARIABLE IMF SLOPE TO FIT THE LCDM PICTURE TO OBSERVED HIGH-Z SUBMILLIMETER SOURCES
Using a Salpeter initial mass function (IMF) allows to describe fairly well a large variety of properties in galaxies. However, some studies have found that it is necessary to change it for a top-heavy IMF in starbursts to give an adequate prediction in the abundance of submillimeter galaxies (SMGs)...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , , , , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2011
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57121297010 |
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