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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 4.

Optical depth and column density in the lower level for the ground state H 2O transitions toward W51. In each panel, the black solid line is inferred from the Gaussian components and the colored dashed line is derived from the interpolated continuum. The optical depth is shown at the native velocity resolution of the spectrum while the column density is shown with a common velocity bin of 0.5 km s −1. The top, middle, and bottom panels show the 556, 1113, and 1669 GHz transitions, respectively.

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