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Shattering of Cosmic Sheets due to Thermal Instabilities: A Formation Channel for Metal-free Lyman Limit Systems

  • Authors: Nir Mandelker, Frank C. van den Bosch, Volker Springel, and Freeke van de Voort

2019 The Astrophysical Journal Letters 881 L20.

  • Provider: AAS Journals

Caption: Figure 2.

Left and center: temperature maps of the system at z = 4, in the same frame as panels (D) and (E) of Figure 1. We show the density-weighted average temperature along the line of sight, integrated over ±400 h−1 ckpc. The accretion shock at the sheet edge is clearly visible in the edge-on view. In the face-on view, the filaments appear cold while the sheet regions have a multiphase structure with hot and cold regions owing to thermal instability. Right: metallicity map in the same frame as the center panel. The filaments are enriched to Z ≳ 10−2Z, while the sheet regions retain Z < 10−3Z. An animation of the temperature evolution from z = 6.84 to z = 2.05, density-weighted in the same edge-on and face-on projections of the large-scale sheet, is available. The left and center panels represent a still frame of the animation at z = 3.93.

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.

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