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        "author": "Steven Rieder",
        "author_email": "steven@rieder.nl",
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            "Development Status :: 4 - Beta",
            "Intended Audience :: Science/Research",
            "License :: OSI Approved :: MIT License",
            "Operating System :: OS Independent",
            "Programming Language :: Python :: 2",
            "Programming Language :: Python :: 2.7",
            "Programming Language :: Python :: 3",
            "Programming Language :: Python :: 3.5",
            "Programming Language :: Python :: 3.6",
            "Programming Language :: Python :: 3.7"
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        "description": "# MASC\nMASC (Make a star cluster) is an AMUSE-based script to generate a star cluster, to be used in N-body simulations or for other purposes. It aims to include all popular distribution models, initial mass functions, and many more features.\n\n## Supported features\n- Stellar distributions: Plummer, King, fractal-based\n- Initial mass function: Salpeter, Kroupa, equal-mass\n- Metallicity\n- Virial ratio\n\n## Not yet supported features\n- Stars in initial binary/triple/multiple configurations\n- Other particles than stars\n\n## Requirements\nMASC requires AMUSE (https://github.com/amusecode/amuse) to work.\n\n## Usage:\nPackage version:\n\n    from amuse.units import units\n    from amuse.ext.masc import new_star_cluster\n    cluster = new_star_cluster(\n        number_of_stars=1024,\n        # stellar_mass=False,\n        initial_mass_function='salpeter',\n        upper_mass_limit=125.0 | units.MSun,\n        effective_radius=3.0 | units.parsec,\n        star_distribution='plummer',\n        # star_distribution_w0=7.0,\n        # star_distribution_fd=2.0,\n        star_metallicity=0.01,\n    )\n\nStandalone version:\n\n    $ python make_a_star_cluster.py -h\n    usage: make_a_star_cluster.py [-h] [-o CLUSTERNAME] [-type FILE TYPE]\n                                  [-N NUMBER_OF_STARS] [-M CLUSTER_MASS]\n                                  [-dist STAR_DISTRIBUTION]\n                                  [-gasdist GAS_DISTRIBUTION]\n                                  [-imf INITIAL_MASS_FUNCTION]\n                                  [-modelnr CLUSTER_MODEL_NUMBER]\n                                  [-kingw KING_PARAMETER_W0]\n                                  [-fractald FRACTAL_PARAMETER_FD]\n                                  [-uml UPPER_MASS_LIMIT] [-Z METALLICITY]\n                                  [-ibf INITIAL_BINARY_FRACTION]\n                                  [-R EFFECTIVE_RADIUS] [-vr VIRIAL_RATIO]\n    \n    optional arguments:\n      -h, --help            show this help message and exit\n      -o CLUSTERNAME        Outputfile name [auto]\n      -type FILE TYPE       Output file type ([amuse]/ascii/starlab/nemo)\n      -N NUMBER_OF_STARS    Number of stars\n      -M CLUSTER_MASS       Cluster mass (takes precedence over number of stars)\n      -dist STAR_DISTRIBUTION\n                            Star distribution ([plummer]/king/fractal)\n      -gasdist GAS_DISTRIBUTION\n                            Gas distribution ([none]/plummer/king/fractal) NOT\n                            IMPLEMENTED YET\n      -imf INITIAL_MASS_FUNCTION\n                            IMF ([kroupa]/salpeter/fixed)\n      -modelnr CLUSTER_MODEL_NUMBER\n                            Model number\n      -kingw KING_PARAMETER_W0\n                            King W0 parameter [7.0]\n      -fractald FRACTAL_PARAMETER_FD\n                            Fractal distribution [2.0]\n      -uml UPPER_MASS_LIMIT\n                            Upper mass limit (in MSun) [125.]\n      -Z METALLICITY        Metallicity [0.01]\n      -ibf INITIAL_BINARY_FRACTION\n                            Initial binary fraction (0-1) [0.] NOT IMPLEMENTED YET\n      -R EFFECTIVE_RADIUS   Cluster radius [3.0] (parsec)\n      -vr VIRIAL_RATIO      Virial ration [0.5], 0.5=stable, 0.75=just expelled\n                            gas, 0.1=collapsing\n\n## COPYRIGHT/LICENSE\nSee LICENSE",
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