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DISTRIBUTION AND MASS OF DIFFUSE AND DENSE CO GAS IN THE MILKY WAY

  • Authors: Julia Roman-Duval, Mark Heyer, Chris Brunt, Paul Clark, Ralf Klessen, and Rahul Shetty

2016 The Astrophysical Journal 818 144.

  • Provider: AAS Journals

Caption: Figure 12.

Average Galactic H2 surface densities of the diffuse (red, detected in 12CO, undetected in 13CO), dense (green, detected in 12CO and 13CO), and very dense (blue, detected in 12CO, 13CO, and CS) components averaged in bins of width 0.1 kpc, as a function of Galactocentric radius in the GRS+UMSB (inner Galaxy only, top), in the EXFC 135–165 survey (outer Galaxy only, middle), and in the EXFC 55–100 survey (inner and outer Galaxy, bottom). In the inner Milky Way covered by the GRS, the pink filled curve indicates the surface density of H2 in molecular clouds identified with a clump finding algorithm in Roman-Duval et al. (2010).

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