2010

H-alpha and Free-Free Emission from the WIM

Dong, Ruobing, Draine, B. T.

Understand

Recent observations have found the ratio of H-alpha to free-free radio continuum to be surprisingly high in the diffuse ionized ISM (the so-called WIM), corresponding to an electron temperature of only ~3000K.

  • Such low temperatures were unexpected in gas that was presumed to be photoionized.
  • We consider a 3-component model for the observed diffuse emission, consisting of a mix of (1) photoionized gas, (2) gas that is recombining and cooling, and (3) cool H I gas.
  • This model can successfully reproduce the observed intensities of free-free continuum, H-alpha, and collisionally-excited lines such as NII 6583.

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