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Dataset . 2019
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Dataset . 2019
License: CC BY
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ZENODO
Dataset . 2019
License: CC BY
Data sources: Datacite
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ZENODO
Dataset . 2019
License: CC BY
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Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity

Research datakeyboard_double_arrow_right Dataset 19 Mar 2019Publisher:Zenodo
Authors: Marchant, Pablo; Langer, Norbert; Podsiadlowski, Philipp; Tauris, Thomas M.; de Mink, Selma; Mandel, Ilya; Moriya, Takashi J.;

doi: 10.5281/zenodo.2891588 , 10.5281/zenodo.2598795 , 10.5281/zenodo.2598794 , 10.5281/zenodo.3431313

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

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.

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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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