We discuss the results of recent 3D simulations of first structure formation in relationship to the formation of the first stars. On the basis of a new, high-resolution AMR simulation (spatial dynamic range = 3 × 10 7), we conclude that the first stars are likely to be massive.
CITATION STYLE
Norman, M. L., Abel, T., & Bryan, G. (2003). First Structure Formation and the First Stars (pp. 250–260). https://doi.org/10.1007/10719504_46
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