Fig. 21 from [Si II], [Fe II], [C II], and H2 Emission from Massive Star‐forming Regions

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[Si II], [Fe II], [C II], and H₂ Emission from Massive Star‐forming Regions

Authors: Michael J. Kaufman, Mark. G. Wolfire, and David J. Hollenbach

Kaufman, Wolfire, & Hollenbach 2006 The Astrophysical Journal 644 283.

Provider: AAS Journals

Caption: Fig. 21.

Relative contributions of PDRs and H II regions to [Si II], [Fe II], and [C II] fine‐structure emission for metal abundances 3 times those in the local diffuse ISM (﹩Z=3﹩). Shown are our model results for ﹩\Phi _{i}=10^{49}﹩ (solid lines) and 10⁵¹ s⁻¹ (dashed lines).

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