Polysulfanes on interstellar grains as a possible reservoir of interstellar sulphur
C. Druard, V. Wakelam

TL;DR
This study investigates the potential role of polysulfanes on interstellar grains as a reservoir of sulphur, using chemical modeling to explore their formation and abundance at different temperatures in dense clouds.
Contribution
The paper introduces new chemical reactions based on recent experiments into the Nautilus gas-grain model, examining sulphur chemistry and the formation of polysulfanes in interstellar environments.
Findings
Polysulfanes are not efficiently produced at 10 K.
At 20 K, H2S on grains decreases in favor of polysulfanes like H2S3.
Sulphur depletion into polysulfanes may occur in slightly warmer regions of interstellar clouds.
Abstract
The form of depleted sulphur in dense clouds is still unknown. Until now, only two molecules, OCS and SO2, have been detected in interstellar ices but cannot account for the elemental abundance of sulphur observed in diffuse medium. Chemical models suggest that solid H2S is the main form of sulphur in denser sources but observational constraints exist that infirm this hypothesis. We have used the Nautilus gas-grain code in which new chemical reactions have been added, based on recent experiments of H2S ice irradiation with UV photons and high energy protons. In particular, we included the new species Sn, H2Sn and C2S. We found that at the low temperature observed in dense clouds, i.e. 10 K, these new molecules are not efficiently produced and our modifications of the network do not change the previous pre- dictions. At slightly higher temperature, 20 K in less dense clouds or in the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
