Articulo
A Variable IMF Slope To Fit The LCDM Picture To Observed High-z Submillimeter Sources
Fecha
2011Registro en:
15010003
WOS:000305259300009
no scielo
eid=2-s2.0-84878321078
Institución
Resumen
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 t