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Molecular Hydrogen Formation Catalyzed by Polycyclic Aromatic Hydrocarbons in the Interstellar Medium

  • Authors: Valéry Le Page, Theodore P. Snow, and Veronica M. Bierbaum

LE PAGE, SNOW & BIERBAUM 2009 The Astrophysical Journal 704 274.

  • Provider: AAS Journals

Caption: Figure 6.

Comparison between observation and the prediction of the model. The general trend of the lowering of the ratio at higher values of n t /χ is well followed by the model. The Orion bar data have been used to scale the other observed data to produce relative values. The values for R are calculated in the fringe of the cloud as in Figure  2. The effect of dust extinction has not been included as discussed in Section 4.1. Error bars are from Habart et al. (2004), except for the Horsehead Nebula (Habart et al. 2005).

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