Observational evidence for rotational desorption of Complex Molecules by radiative torques from Orion BN/KL
Le Ngoc Tram, Hyeseung Lee, Thiem Hoang, Joseph M. Michail, David T., Chuss, Sarah Nickerson, Naseem Rangwala, William T. Reach

TL;DR
This study provides observational evidence that radiative torques can cause rotational desorption of complex organic molecules in star-forming regions, explaining their presence at lower temperatures than previously thought.
Contribution
It demonstrates the role of radiative torque-induced rotational desorption in releasing COMs at low temperatures, supported by ALMA observations and polarization data analysis.
Findings
COMs detected at temperatures below 100 K.
Polarization degree decreases with increasing dust temperature.
Observational support for rotational desorption mechanism.
Abstract
Complex Organic Molecules (COMs) are believed to form in the ice mantle of dust grains and are released to the gas by thermal sublimation when grain mantles are heated to temperatures of . However, some COMs are detected in regions with temperatures below 100 K. Recently, a new mechanism of rotational desorption due to centrifugal stress induced by radiative torques (RATs) is proposed by Hoang & Tram 2020 that can desorb COMs at low temperatures. In this paper, we report observational evidence for rotational desorption of COMs toward the nearest massive star-forming region Orion BN/KL. We compare the abundance of three representative COMs which have very high binding energy computed by the rotational desorption mechanism with observations by ALMA, and demonstrate that the rotational desorption mechanism can explain the existence of such COMs. We also analyze…
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.
