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High Spectral Resolution Observations toward Orion BN at 6 μm: No Evidence for Hot Water

  • Authors: Nick Indriolo, Jonathan Tan, A. C. A. Boogert, C. N. DeWitt, E. J. Montiel, D. A. Neufeld, and M. J. Richter

2018 The Astrophysical Journal Letters 865 L18.

  • Provider: AAS Journals

Caption: Figure 2.

Spectra showing the water absorption lines observed toward BN. Fits to the components at 8, 0.5, and −17 km s−1, are shown by blue, cyan, and green curves, respectively, and the sum of all components is shown as a red dashed curve. The top spectrum shows a non-detection of the transition predicted to have the strongest absorption after the detected transitions in the observed wavelength range (ν2 31,2–22,1 at 6.1068262 μm). Spectra have been shifted vertically for clarity.

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