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The Cosmic-Ray Ionization Rate in the Galactic Disk, as Determined from Observations of Molecular Ions

  • Authors: David A. Neufeld, and Mark G. Wolfire

2017 The Astrophysical Journal 845 163.

  • Provider: AAS Journals

Caption: Figure 6.

Estimates of ﹩{\zeta }_{p}({\rm{H}})﹩, derived from measurements of the H2 and ﹩{{\rm{H}}}_{3}^{+}﹩ column densities, as a function of the measured ﹩N({{\rm{H}}}_{2})﹩ (top panel) and of the derived ﹩{A}_{{\rm{V}}}(\mathrm{tot})﹩ (bottom panel). Black diamonds: measurements obtained from direct observations of H2. Magenta diamonds: measurements in which the H2 column densities have been inferred indirectly from observations of CH or ﹩E(B-V)﹩. Dashed red lines: best fits to all the data.

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