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Thermal Phases of the Neutral Atomic Interstellar Medium from Solar Metallicity to Primordial Gas
2019 The Astrophysical Journal 881 160.
Caption: Figure 5.
Cooling (left) and heating (right) rates per hydrogen nucleus (erg s−1), as functions of the gas hydrogen density, at various metallicities.
© 2019. The American Astronomical Society. All rights reserved.
