Pablo Marchant
2018-10-27
<p>Models of pulsational pair-instability supernovae arising from the evolution of metal poor helium stars. These simulations have been made with the MESA software instrument for stellar evolution, and are used in the paper <a href="https://ui.adsabs.harvard.edu/abs/2019ApJ...882...36M/abstract">"Pulsational pair-instability supernovae in very close binaries"</a>. Data includes machine-readable tables, both history and profile files from the simulations, as well as the terminal output and a movie for each. All MESA output files have been post-processed to reduce their size. All the code used to process the MESA simulations and produce figures is provided in a jupyter-notebook.</p>
<p>WARNING: Simulations were done using a development MESA version (11123) rather than an official release. </p>
<p>List of files:</p>
<p>- template.tar.xz: MESA work folder to reproduce the simulations.</p>
<p>- xxx_xx.tar.xz: Each of these files contains stellar profiles at different moments of evolution for one simulation.</p>
<p>- histories.tar.xz: MESA history files for each simulation, containing the time evolution of quantities that are single-valued at each moment in time.</p>
<p>- preSN.tar.xz: profiles for stars before the onset of pulsations (see paper for definition).</p>
<p>- movies.tar: Movies for all simulations, produced using MESAs pgstar.</p>
<p>- terminal_output.tar.xz: Terminal output from the simulations.</p>
<p>- masses_table.txt: Machine readable version of Table 1 in the paper.</p>
<p>- pulse_tables.tar.xz: machine readable tables containing mass lost, time, and kinetic energy of each pulse.</p>
<p>- notebook.tar.xz: jupyter-notebook plus complementary files used to post-process the data and produce Figures.</p>
<p>This version of the files has an updated notebook.tar.xz to produce the figures in the published version of the paper.</p>
https://doi.org/10.5281/zenodo.3786599
oai:zenodo.org:3786599
eng
Zenodo
https://doi.org/10.3847/1538-4357/ab3426
https://zenodo.org/communities/mesa
https://doi.org/10.5281/zenodo.1211427
info:eu-repo/semantics/openAccess
Creative Commons Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/legalcode
The Astrophysical Journal, 882(1), article id. 36, (2018-10-27)
PPISN
PISN
stellar evolution
black hole
gravitational waves
supernova
binary star
Pulsational pair-instability supernovae in very close binaries
info:eu-repo/semantics/other