Figure 11 from SIMULATIONS OF THE CHEMISTRY IN THE SMALL MAGELLANIC CLOUD

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SIMULATIONS OF THE CHEMISTRY IN THE SMALL MAGELLANIC CLOUD

Authors: Kinsuk Acharyya, and Eric Herbst

2016 The Astrophysical Journal 822 105.

Provider: AAS Journals

Caption: Figure 11.

CH₃OH gas-phase abundance as a function of time for various values of grain temperature, with A_V = 10 (Panel (a)) and 5 mag (Panel (b)) for n_H = 1 × 10⁵ cm⁻³.

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