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Code to run the simulations and generate figures of the paper: "External photoevaporation of circumstellar disks constrains the timescale for planet formation" (2019MNRAS.490..5678C)

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2019MNRAS.490..5678C External photoevaporation of circumstellar disks constrains the timescale for planet formation

Francisca Concha-Ramírez, Martijn J. C. Wilhelm, Simon Portegies Zwart, Thomas J. Haworth

DOI License: GPL v3 python

(Code to run the simulations and generate figures of the paper: 2019MNRAS.490..5678C External photoevaporation of circumstellar disks constrains the timescale for planet formation.)

For questions please contact Francisca Concha-Ramírez, fconcha at strw.leidenuniv.nl

Getting Started

Requisites

Running the simulations

You can run an individual simulation by using the AMUSE script directly:

amuse.sh vader_cluster.py

The script has extensive options which can be passed through the command line. For a list of these options run:

amuse.sh vader_cluster.py --help

Creating the plots

All figures of the paper (except Figures 3 and 4, which are flow charts) were created using the script plots.py:

amuse.sh plots.py

A list of options is available for this script, including the path to the files that you want to use for the plots. To see the list of options add --help or -h to the line above.

The tests and figures of the appendix can be created using the script tests.py:

amuse.sh tests.py

License

This project is licensed under the GPL v3 License - see the LICENSE.md file for details

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Code to run the simulations and generate figures of the paper: "External photoevaporation of circumstellar disks constrains the timescale for planet formation" (2019MNRAS.490..5678C)

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