http://arxiv.org/abs/1709.06647
Using cosmological volume simulations and a custom built sub-grid model for Pop III star formation, we examine the baseline dust extinction in the first galaxies due to Pop~III metal enrichment in the first billion years of cosmic history. We find that while the most enriched, high-density lines of sight in primordial galaxies can experience a measurable amount of extinction from Pop III dust ($E(B-V){\rm max}=0.07,\ A{\rm V,max}\approx0.28$), the average extinction is very low with $\left< E(B-V) \right> \lesssim 10^{-3}$. We derive a power-law relationship between dark matter halo mass and extinction of $E(B-V)\propto M_{\rm halo}^{0.80}$. Performing a Monte Carlo parameter study, we establish the baseline reddening of the UV spectra of dwarf galaxies at high redshift due to Pop III enrichment only. With this method, we find $\left<\beta_{\rm UV}\right>-2.72\pm0.12$, which is both nearly halo mass and redshift independent.
J. Jaacks, S. Finkelstein and V. Bromm
Thu, 21 Sep 17
32/50
Comments: 6 pages, 5 figures