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Sub-parsec resolution cosmological simulations of star-forming clumps at high redshift with feedback of individual stars

By Francesco Calura and others
We introduce a new set of zoom-in cosmological simulations with sub-pc resolution, intended to model extremely faint, highly magnified star-forming stellar clumps, detected at z=6.14 thanks to gravitational lensing. The simulations include feedback from individual massive stars (in both the pre-supernova and supernova phases), generated via stochastic, direct sampling of... Show more
August 16, 2022
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Sub-parsec resolution cosmological simulations of star-forming clumps at high redshift with feedback of individual stars
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