Shock-type inference of L1157 B2 using methanol desorption
Cedric Baijot, Maria Groyne, Micha\"el De Becker

TL;DR
This study uses methanol desorption in shock models to diagnose the shock type of L1157 B2, successfully distinguishing it as a non-irradiated C-type shock through comparison with observations and benchmarks.
Contribution
It introduces a method based on methanol desorption percentages to differentiate shock types in non-irradiated regions, validated on L1157 B2.
Findings
L1157 B2 is identified as a non-irradiated C-type shock.
Methanol desorption percentage effectively distinguishes shock types.
The method shows good applicability in shock diagnostics.
Abstract
Shock types of low-velocity molecular outflows are not always well constrained. Astrochemical comparisons are often made between low-velocity and high-velocity outflows, but without considering the question of the shock type. We investigated molecular abundances of post-shock regions to determine whether strong differences between non-irradiated C-type and J-type shocks can be highlighted. One of the main application goals is to diagnose the shock type of the protostellar object L1157 B2 through the use of molecular tracers. We simulated grid sets of shock models with the Paris-Durham Shock code with velocities ranging from 5 to 19 km/s and low densities from to cm. We computed the desorption percentage of methanol in these simulations and estimated it at higher velocities. We compared our results to observational measurements of L1157 B2 and with a benchmark of…
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.
Taxonomy
TopicsAstrophysics and Star Formation Studies · Astro and Planetary Science · High-pressure geophysics and materials
