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)...
Tallennettuna:
| Julkaisussa: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Päätekijät: | , , , , , |
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
Universidad Nacional Autónoma de México
2011
|
| Aiheet: | |
| Linkit: | https://www.redalyc.org/articulo.oa?id=57121297010 |
| Tagit: |
Ei tageja, Lisää ensimmäinen tagi!
|