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EARLY STRUCTURE FORMATION FROM PRIMORDIAL DENSITY FLUCTUATIONS WITH A BLUE, TILTED POWER SPECTRUM

  • Authors: Shingo Hirano, Nick Zhu, Naoki Yoshida, David Spergel, and Harold W. Yorke

2015 The Astrophysical Journal 814 18.

  • Provider: AAS Journals

Caption: Figure 3.

Projected densities for dark matter (Panel (a)) and baryonic components (b). We also plot the projected gas temperature (c) at the formation sites of the primordial stars ID 300 (top; zform = 46) and ID 313 (bottom; zform = 186). The plotted region has a proper 100 pc on a side. We scale the density in units of particle number density per cubic-centimeter.

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