Azimuthal C/O Variations in a Planet-Forming Disk

DALI physical-chemical disk models presented in 'Azimuthal C/O Variations in a Planet-Forming Disk' (Keyte et al. 2023).

There are two individual models included here. The 'baseline' model is used to produce outputs for the region of the disk where C/O=0.5. The 'elevated' model is used to produce outputs for the regions of the disk where C/O=1.5.

The baseline model can be run in the normal way, but the outputs themselves are already included in the folder.

The 'elevated' model will not run in the regular way. The source code has been edited so that it can take in the abundances from a previous run as the starting point for the chemistry (in the form of an out.dat style table). The outputs are already included, but should you want to rerun the model yourself, follow the steps in the readme file within the folder.

The final 'composite' model presented in the paper is created by splicing together the outputs (as described in Keyte et al. 2023). This is achieved using a custom Python script, please contact me if you would like to use this.