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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 2.

Energy level diagram for ortho and para water. The transitions within the HIFI spectral coverage are indicated by solid lines, while those outside of this range are indicated by dashed lines. The transitions observed in PRISMAS are indicated by heavy lines, labeled with the frequency of H 2 16O and H 2 18O (in italics) when observed.

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