Dataset for: "Modeling the Hα Emission Surrounding Spica using the Lyman Continuum from a Gravity-darkened Central Star"
收藏资源简介：
<strong>Summary: </strong>This deposit supplements the manuscript, "<em>Modeling the Hα Emission Surrounding Spica using the Lyman Continuum from a Gravity-darkened Central Star</em>", 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<br> example_cloudy_input_file.txt Cloudy script<br> spica_i=100_V5_solar.ascii Spica input stellar spectral energy distribution<br> spica_i=110_V5_solar.ascii Spica input stellar spectral energy distribution<br> spica_i=116_V5_solar.ascii Spica input stellar spectral energy distribution<br> spica_i=120_V5_solar.ascii Spica input stellar spectral energy distribution<br> spica_i=130_V5_solar.ascii Spica input stellar spectral energy distribution<br> spica_i=140_V5_solar.ascii Spica input stellar spectral energy distribution<br> spica_i=150_V5_solar.ascii Spica input stellar spectral energy distribution<br> spica_i=160_V5_solar.ascii Spica input stellar spectral energy distribution<br> spica_i=170_V5_solar.ascii Spica input stellar spectral energy distribution<br> spica_i=180_V5_solar.ascii Spica input stellar spectral energy distribution<br> spica_i=90_V5_solar.ascii Spica input stellar spectral energy distribution<br> <strong>System requirements:</strong> The input script and SED files correspond to Cloudy code version 17.02:<br> Codebase: https://trac.nublado.org/<br> Primary documentation: Ferland et al. (2017RMxAA..53..385F; arXiv:1705.10877)<br> Additional documentation provided in the ReadMe file.
