FIRST Project: Formation and Feedback of the First Stars

Computer Science

Scientific paper

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Population Iii Stars, Hii Regions, Emission And Reflection Nebulae, Star Formation, Hydrodynamics

Scientific paper

We introduce the ``FIRST Project'', where high-resolution 3D radiation hydrodynamic simulations of first star formation are performed with a newly developed dedicated computer having a peak speed of 36.1 Tflops. By solving the hydrodynamics consistently with the radiative transfer of UV radiation from first stars, we explore the radiation hydrodynamic feedback in first generation objects, and consider the star formation efficiency of the first stars.

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