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 Journal839107.
Provider: AAS Journals
Caption: Figure 8.
Histograms of the thermal pressure of the diffuse ISM of the LMC and SMC derived in Section 4.3.