Dataset for: "Modeling the Hα Emission Surrounding Spica using the Lyman Continuum from a Gravity-darkened Central Star"

Summary: This deposit supplements the manuscript, "Modeling the Hα Emission Surrounding Spica using the Lyman Continuum from a Gravity-darkened Central Star", accepted to the Astrophysical Journal. The tar.gz archive file contains an example Cloudy script and associated data. The complete listing of the files included in this archive file are given here:  

    ReadMe                                          Documentation file
    example_cloudy_input_file.txt        Cloudy script
    spica_i=100_V5_solar.ascii            Spica input stellar spectral energy distribution
    spica_i=110_V5_solar.ascii            Spica input stellar spectral energy distribution
    spica_i=116_V5_solar.ascii            Spica input stellar spectral energy distribution
    spica_i=120_V5_solar.ascii            Spica input stellar spectral energy distribution
    spica_i=130_V5_solar.ascii            Spica input stellar spectral energy distribution
    spica_i=140_V5_solar.ascii            Spica input stellar spectral energy distribution
    spica_i=150_V5_solar.ascii            Spica input stellar spectral energy distribution
    spica_i=160_V5_solar.ascii            Spica input stellar spectral energy distribution
    spica_i=170_V5_solar.ascii            Spica input stellar spectral energy distribution
    spica_i=180_V5_solar.ascii            Spica input stellar spectral energy distribution
    spica_i=90_V5_solar.ascii              Spica input stellar spectral energy distribution

System requirements: The input script and SED files correspond to Cloudy code version 17.02:
        Codebase: https://trac.nublado.org/
        Primary documentation: Ferland et al. (2017RMxAA..53..385F; arXiv:1705.10877)

Additional documentation provided in the ReadMe file.