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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. 8.

H2 0–0 S(1)/0–0 S(0) line intensity ratio as a function of hydrogen nucleus density n and FUV radiation field G0.

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