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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 1.

Images showing the H0 column density map (blue; Stanimirovic et al. 1999; Kim et al. 2003), Herschel 160 μm continuum emission (red; Meixner et al. 2013), and MAGMA CO line emission (green; Wong et al. 2011; E. Muller et al. 2017, in preparation) in the LMC (top) and SMC (bottom). The white circles denote the positions studied in this paper. The size of the circles does not denote the beam size employed in any of the observations presented here.

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