Figure 10 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 10.

Sample comparison between the [C I] ﹩{{}^{3}{\rm{P}}}_{2}\to {}^{3}{{\rm{P}}}_{1}/{{}^{3}{\rm{P}}}_{1}\to {}^{3}{{\rm{P}}}_{0}﹩ line intensity ratio and the peak intensity of the [C I] ﹩{{}^{3}{\rm{P}}}_{1}\to {}^{3}{{\rm{P}}}_{0}﹩ line with the grid of RADEX models. The comparison is shown at the kinetic temperature at which the minimum value of ﹩{\chi }^{2}﹩ is found.

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