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. Author manuscript; available in PMC: 2016 Jun 6.
Published in final edited form as: Astron Astrophys. 2016 May;589:A60. doi: 10.1051/0004-6361/201527089

Fig. 7.

Fig. 7

Chemical model abundance results. Predicted CO, H2CO, and SO fractional abundances as a function of time for different molecular hydrogen densities, gas-to dust mass ratios, and grain sizes.