Figure 9 from Water Absorption in Galactic Translucent Clouds: Conditions and History of the Gas Derived from Herschel/HIFI PRISMAS Observations

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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 9.

Total column density of water as a function of the column density of molecular hydrogen and hydrogen nuclei. (a) The red solid line is the best linear fit to the data. (b) The red solid line is the best linear fit to the data. Arrows show the features for which we only have a lower limit for N _H.

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