SIMULATIONS OF THE CHEMISTRY IN THE SMALL MAGELLANIC CLOUD
Authors: Kinsuk Acharyya, and Eric Herbst
2016 The Astrophysical Journal822105.
Provider: AAS Journals
Caption: Figure 2.
Variation of gas-phase CO abundance as a function of grain temperature at various times for AV = 10 (Figure 2(a)) and 5 mag (Figure 2(b)) for nH = 1 × 105 cm−3.
