SIMULATIONS OF THE CHEMISTRY IN THE SMALL MAGELLANIC CLOUD
Authors: Kinsuk Acharyya, and Eric Herbst
2016 The Astrophysical Journal822105.
Provider: AAS Journals
Caption: Figure 1.
Gaseous CO abundance as a function of time for various values of grain temperature, with AV = 10 (Panel (a)) and 5 mag (Panel (b)) for nH = 1 × 105 cm−3.