IMF of pop III stars

Details IMF of pop III stars IMF of pop III stars

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009rmxac..35s.303p&link_type=abstract

XII Latin American IAU Regional Meeting (Eds. G. Magris, G. Bruzual, & L. Carigi) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Scientific paper

I performed a perturbation analysis of matter's overdensity in high redshift halos in order to know the distribution in size of objects that can collapse at first. In order to see which objects can form stars, I performed an analysis of the molecular cooling inside the first formed structures. This analysis gives a possible IMF for the first stars in the Universe.

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