Stratified Distribution of Organic Molecules at the Planet-Formation Scale in the HH 212 Disk Atmosphere
Chin-Fei Lee, Claudio Codella, Cecilia Ceccarelli, and Ana, Lopez-Sepulcre

TL;DR
This study maps and analyzes the distribution of organic molecules in the HH 212 disk atmosphere, revealing stratification and formation mechanisms relevant to prebiotic chemistry in planet-forming regions.
Contribution
It provides the first detailed spatial distribution and formation insights of formamide and related molecules in a protostellar disk at Solar-System scales.
Findings
Molecules show stratified distribution with increasing outer radius correlating with decreasing binding energy.
H2CO's extended distribution and different kinematics suggest it is unlikely a direct parent of NH2CHO.
HNCO likely acts as a daughter species of desorbed NH2CHO.
Abstract
Formamide (NH2CHO) is considered an important prebiotic molecule because of its potential to form peptide bonds. It was recently detected in the atmosphere of the HH 212 protostellar disk on the Solar-System scale where planets will form. Here we have mapped it and its potential parent molecules HNCO and H2CO, along with other molecules CH3OH and CH3CHO, in the disk atmosphere, studying its formation mechanism. Interestingly, we find a stratified distribution of these molecules, with the outer emission radius increasing from ~ 24 au for NH2CHO and HNCO, to 36 au for CH3CHO, to 40 au for CH3OH, and then to 48 au for H2CO. More importantly, we find that the increasing order of the outer emission radius of NH2CHO, CH3OH, and H2CO is consistent with the decreasing order of their binding energies, supporting that they are thermally desorbed from the ice mantle on dust grains. We also find…
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