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The fate of formamide in a fragmenting protoplanetary disk

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Figure

Table 1
Figure 1. Gas-phase abundance of NHacross phase 12CHO (formamide), CO, H2O, NH2, and H2CO across the pre-disk phases in our chemical modeling
Figure 3. Evolution of the total column density of the disk (gray scale) overlaid with the snowlines of CO (red), NH2CHO (green), and H2O (blue)
Figure 4. Median abundance of formamide in the gas phaserepresents a different time, comprised between the formation and destruction time (full lines) and on the grain surface (dashed lines) as a function of the radius of each fragment: John (topleft), Pau
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