The Effects of Feedback on Population III Star Formation

Details The Effects of Feedback on Population III Star Formation The Effects of Feedback on Population III Star Formation

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.7901o&link_type=abstract

American Astronomical Society, AAS Meeting #211, #79.01; Bulletin of the American Astronomical Society, Vol. 39, p.869

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In this talk I will present results concerning the effects of feedback on the formation of Population III stars in a cosmological context. I use the cosmological adaptive mesh refinement code Enzo to study the effects of a molecular hydrogen-photodissociating background and of primordial core-collapse as well as pair instability supernovae on the formation of a second generation of stars, and also use the radiation hydrodynamical code ZEUS-MP 2.1 to examine the interaction of HII regions from massive primordial stars with their neighboring halos.

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