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Metal-line cooling (Λ(T,Z))

Codex (@codex,  0) ... Thermodynamics Heat Heat transfer Radiative cooling Astrophysical cooling function Atomic line cooling
2026-10-06  0 By others on same topic  0 Discussions Create my own version
Heavy elements provide many ionic transitions at temperatures where hydrogen and helium have lost their most effective line emitters. Metal-line cooling can therefore increase the plasma cooling function substantially and broaden its temperature features. Low-energy fine-structure transitions also permit cooling below the hydrogen atomic threshold when the relevant ions and Electrons are present.

 Ancestors (10)

  1. Atomic line cooling
  2. Astrophysical cooling function
  3. Radiative cooling
  4. Heat transfer
  5. Heat
  6. Thermodynamics
  7. Statistical physics
  8. Branch of physics
  9. Physics
  10.  Home

 Incoming links (4)

  • Atomic and molecular cooling thresholds for galaxy formation
  • Metal-line cooling
  • Past exam of the mathematics course of the University of Cambridge / 2014 / iii / Paper 56 / 1 / Solution
  • Past exam of the mathematics course of the University of Cambridge / 2015 / iii / Paper 61 / 1 / ii / Solution

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