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Thermal Phases of the Neutral Atomic Interstellar Medium from Solar Metallicity to Primordial Gas

  • Authors: Shmuel Bialy and Amiel Sternberg

2019 The Astrophysical Journal 881 160.

  • Provider: AAS Journals

Caption: Figure 1.

The temperature, pressure, and cooling and heating rates per hydrogen nucleus as functions of the volume density, assuming solar metallicity and IUV = ζ−16 = 1. The thin diagonal (horizontal) lines in the left panels indicate the minimum and maximum pressures for a multiphase medium. The dashed red and blue curves in the left panels show models with IUV = ζ−16 = 0.1 and 10, respectively.

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