| Issue |
A&A
Volume 705, January 2026
|
|
|---|---|---|
| Article Number | A185 | |
| Number of page(s) | 15 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/202553978 | |
| Published online | 22 January 2026 | |
Shock-type inference of L1157 B2 using methanol desorption
Space Sciences, Technologies and Astrophysics Research (STAR) Institute, University of Liège,
Quartier Agora, 19c, Allée du 6 Août, B5c,
4000
Sart Tilman,
Belgium
★ Corresponding author: This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
31
January
2025
Accepted:
11
November
2025
Context. 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.
Aims. 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.
Methods. 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 102 to 105 cm−3. 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 four already identified shocks.
Results. L1157 B2 has been diagnosed as a non-irradiated C-type shock, and the method showed a good applicability through the benchmark. Methanol formed in the icy mantle of grains can serve to trace the differences between shock types, at least in non-irradiated conditions. A requirement for the applicability of a species as a shock-type tracer is that it does not undergo significant enhancement or destruction, but is mainly impacted by desorption processes under shocked conditions.
Conclusions. The desorption percentage of methanol is a good criterion in characterizing the shock type of L1157 B2 and should be investigated as a general method to diagnose the shock type in non-irradiated regions. We identify L1157 B2 as a non-irradiated C-type shock with velocities and densities fitting with previous studies.
Key words: astrochemistry / molecular processes / shock waves / methods: numerical / ISM: molecules
© The Authors 2026
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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