869 citations · 7.6k across the 94 of their papers we have counts for
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Amplification of Magnetic Fields in a Primordial HII Region and Supernova
Daegene Koh, John H. Wise
Magnetic fields permeate the Universe on all scales and play a key role during star formation. We study the evolution of magnetic fields around a massive metal-free (Population III…
X-ray Background at High Redshifts from Pop III Remnants: Results from Pop III star formation rates in the Renaissance Simulations
Hao Xu, Kyungjin Ahn, Michael L Norman +2
Due to their long mean free paths, X-rays are expected to have many significant impacts globally on the properties of the intergalactic medium (IGM) by their heating and ionizing p…
Late Pop III Star Formation During the Epoch of Reionization: Results from the Renaissance Simulations
Hao Xu, Michael L. Norman, Brian W. O'Shea +1
We present results on the formation of Pop III stars at redshift 7.6 from the Renaissance Simulations, a suite of extremely high-resolution and physics-rich radiation transport hyd…
Galaxy Properties and UV Escape Fractions During Epoch of Reionization: Results from the Renaissance Simulations
Hao Xu, John H. Wise, Michael L. Norman +2
Cosmic reionization is thought to be primarily fueled by the first generations of galaxies. We examine their stellar and gaseous properties, focusing on the star formation rates an…
Positive or Negative? The Impact of X-ray Feedback on the Formation of Direct Collapse Black Hole Seeds
John A. Regan, Peter H. Johansson, John H. Wise
A nearby source of Lyman-Werner (LW) photons is thought to be a central component in dissociating H and allowing for the formation of a direct collapse black hole seed. Nearby…