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Research data . Dataset . 2019

Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity

Marchant, Pablo; Langer, Norbert; Podsiadlowski, Philipp; Tauris, Thomas M.; de Mink, Selma; Mandel, Ilya; Moriya, Takashi J.;
Open Access
Abstract
MESA inlists, run_star_extras, and data associated with Marchant et al. (2017). MESA version 8118. Publication DOI: 10.1051/0004-6361/201630188 Files are also available in a gihub repository here 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. The file summary_tables.tar.gz contains summarized information for each simulation in ascii format.
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