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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 1.

Subsets of the observed spectra of MonR2 IRS3 with the best-fit local thermodynamic equilibrium (LTE) model plotted in red; telluric transmission is plotted in blue. Data are plotted in the rest frame of MonR2 IRS3 (VLSR = 10 km s−1). For the best-fit parameters and their definitions, see Section 3.1. We use the upper limit Doppler parameter (3.20 km s−1) in generating the plotted model. Gaps in the data represent regions where the telluric transmission drops below 80%. Blue stars denote absorption features due H2O in the target.

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