Image Details

Choose export citation format:

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 8.

Ratios between the computed abundances of gas-phase CO (a), CH3OH (b), H2CO (c), N2 (d), NH3 (e), and HCN (f) in the Milky Way and in the SMC are plotted vs. time at grain temperatures at 10 and 30 K. The dashed horizontal line indicates the ratio of the elemental abundance of carbon ((a), (b), (c)) and nitrogen ((d), (e), (f)) between the two galaxies. The closely spaced abundance ratios of carbon and oxygen appear as one line.

Other Images in This Article

Show More

Copyright and Terms & Conditions