Fig. 13 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. 13.

H₂ 0–0 S(1) line intensity as a function of hydrogen nucleus density n and FUV radiation field G₀, for models with metal abundances increased by a factor of 3.

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