Figure 4 from Characterizing the Transition from Diffuse Atomic to Dense Molecular Clouds in the Magellanic Clouds with [C II], [C I], and CO

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Characterizing the Transition from Diffuse Atomic to Dense Molecular Clouds in the Magellanic Clouds with [C II], [C I], and CO

Authors: Jorge L. Pineda, William D. Langer, Paul F. Goldsmith, Shinji Horiuchi, Thomas B. H. Kuiper, Erik Muller, Annie Hughes, Jürgen Ott, Thangasamy Velusamy, and Tony Wong

2017 The Astrophysical Journal 839 107.

Provider: AAS Journals

Caption: Figure 4.

Sample [C II] and [C I] ³P﹩{}_{2}{-}^{3}﹩P₁ spectrum illustrating the decomposition between [C II] emission associated with PDRs, CO-dark H₂ gas, cold H I, and ionized gas. See Section 3 for details on the decomposition of the [C II] emission.

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