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Water Absorption in Galactic Translucent Clouds: Conditions and History of the Gas Derived from Herschel/HIFI PRISMAS Observations

  • Authors: N. Flagey, P. F. Goldsmith, D. C. Lis, M. Gerin, D. Neufeld, P. Sonnentrucker, M. De Luca, B. Godard, J. R. Goicoechea, R. Monje, and T. G. Phillips

Flagey et al. 2013 The Astrophysical Journal 762 11.

  • Provider: AAS Journals

Caption: Figure 6.

Comparison between the column density of the 1 01 level inferred from the 556 GHz transition ( ) and the 1669 GHz transition ( ). Each data point represents one absorption Gaussian profile. In each panel, the red solid line is the best linear fit to the data, the blue dashed line is a column density ratio equal to unity, and the orange dashed line is the average column density ratio.

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