Abstract
We study the formation of primordial proto-stars in a ACDM universe using ultra high-resolution cosmological simulations. Our approach includes all the relevant atomic and molecular physics to follow the thermal evolution of a prestellar gas cloud to "stellar" densities. We describe the numerical implementation of the physics. We also show the result of a simulation of the formation of primordial stars in a reionized gas. © 2008 International Astronomical Union.
Author supplied keywords
Cite
CITATION STYLE
Yoshida, N. (2008). Protostar formation in the early universe. In Proceedings of the International Astronomical Union (Vol. 4, pp. 18–23). Cambridge University Press. https://doi.org/10.1017/S1743921308024538
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.
