Open Access
Table 5
Summary of the simulation setups discussed in this work.
| Model | Description |
|---|---|
| L1544 | |
| KC | Constant abundance throughout the core with a drop to zero in the central 1500au, applied to the Keto-Caselli model for L1544 (Keto et al. 2015) |
| STKC | Abundance profile derived with a static physical model adopting the parameters and physical structure of the Keto-Caselli model for L1544 |
| HD | Constant abundance throughout the core with a drop to zero in the central 1500 au, applied to the HDCRT model for L1544 |
| STHD | Abundance profile derived with a static physical model adopting the parameters and physical structure of the HDCRT model for L1544 |
| HD0 | Abundance profile derived from the best match between the Keto-Caselli and the fiducial hydrodynamical model presented in Sipilä et al. (2022) |
| HH211 | |
| const | Constant abundance throughout the core, applied to the physical model for HH211 derived in this work |
| 2-phase | Abundance profile derived with a static physical model adopting the parameters and physical structure of the physical model for HH211 derived in this work, applying the 2-phase model of the chemical code (= gas phase chemistry and entire ice on the grains are active) |
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