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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 9.

Sample comparison between the observed CO and 13CO line ratios and the predictions from the RADEX model. The lines represent the observed line ratios ± the uncertainties in their determination. The comparisons are shown at the kinetic temperature at which the minimum value of ﹩{\chi }_{\mathrm{total},\min }^{2}﹩ is located. In the middle and lower panels, we show cases in which the 3σ upper limit of the 13CO ﹩J=1\to 0{/}^{12}\mathrm{CO}﹩ ﹩J=1\to 0﹩ and/or the 12CO ﹩J=7\to 6/J=3\to 2﹩ ratios are used to discard solutions.

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