Figure 2 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 2.

Sample spectra of ionic, atomic, and molecular species in the LMC and SMC. We show examples of diffuse regions and dense PDRs. The shaded region in the H I spectra represents the velocity range where we assume that the H I emission is in the form of CNM (see Section 3.2).

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