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High-resolution SOFIA/EXES Spectroscopy of SO2 Gas in the Massive Young Stellar Object MonR2 IRS3: Implications for the Sulfur Budget

  • Authors: Ryan Dungee, Adwin Boogert, Curtis N. DeWitt, Edward Montiel, Matthew J. Richter, Andrew G. Barr, Geoffrey A. Blake, Steven B. Charnley, Nick Indriolo, Agata Karska, David A. Neufeld, Rachel L. Smith, and Alexander G. G. M. Tielens

2018 The Astrophysical Journal Letters 868 L10.

  • Provider: AAS Journals

Caption: Figure 2.

Isolated absorption features from each of our data sets showing line width comparisons. The best-fit model is plotted in red. Note that the b = 3.20 km s−1 used for SO2 here is an upper limit for the intrinsic line width. For the best-fit parameters and their definitions, see Section 3.1. Panels (a) and (b) are isolated absorption features from the SO2 and 13CO spectra, respectively. Panels (c) and (d) are of the same SO2 absorption feature, one convolved to the same resolution as our 13CO data. The point with error bars represents the typical uncertainty for the observed spectra in that panel.

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