Dataset Open Access
Marchant, Pablo;
Langer, Norbert;
Podsiadlowski, Philipp;
Tauris, Thomas M.;
de Mink, Selma;
Mandel, Ilya;
Moriya, Takashi J.
{ "publisher": "Zenodo", "DOI": "10.5281/zenodo.3431313", "container_title": "Astronomy & Astrophysics", "title": "Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity", "issued": { "date-parts": [ [ 2019, 3, 19 ] ] }, "abstract": "<p>MESA inlists, run_star_extras, and data associated with <a href=\"https://ui.adsabs.harvard.edu/?#abs/2017A&A...604A..55M\">Marchant et al. (2017)</a>. MESA version 8118.</p>\n\n<p>Publication DOI: <a href=\"https://doi.org/10.1051/0004-6361/201630188\">10.1051/0004-6361/201630188</a></p>\n\n<p>Files are also available in a gihub repository <a href=\"https://github.com/orlox/mesa_input_data/tree/master/2016_ULX\">here</a></p>\n\n<p>Upload includes post-processed simulation output in the files Z-XX.tar.xz, where XX represents the metallicity (Z-25.tar.gz is for a metallicity of log10(Z)=-2.5). Each folder inside the archive corresponds to a single MESA simulation, with the name indicating the value of log10(M_1), q=M2/M1 and the orbital period in days. For example, the directory 1.600_0.500_0.900 corresponds to the simulation with log10(M1/Msun)=1.6, M2/M1=0.5 and Porb=0.9 days. Each folder is also a MESA template folder, containing all input files neccesary to reproduce that individual simulation.</p>\n\n<p>The file summary_tables.tar.gz contains summarized information for each simulation in ascii format.</p>", "author": [ { "family": "Marchant, Pablo" }, { "family": "Langer, Norbert" }, { "family": "Podsiadlowski, Philipp" }, { "family": "Tauris, Thomas M." }, { "family": "de Mink, Selma" }, { "family": "Mandel, Ilya" }, { "family": "Moriya, Takashi J." } ], "page": "id.A55, 34 pp. (2017)", "volume": "Volume 604", "version": "8845", "type": "dataset", "id": "3431313" }
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