September 12, 2019 Journal article Open Access

Renzo, M.; Farmer, R.; Justham, S.; Gotberg, Y.; de Mink,. S. E.; Zapartas, E.; Marchant, P.; Smith, N.

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{
  "inLanguage": {
    "alternateName": "eng", 
    "@type": "Language", 
    "name": "English"
  }, 
  "description": "<p>Numerical results of the simulations presented in Renzo, Farmer, et al. 2020 (https://ui.adsabs.harvard.edu/abs/2020arXiv200205077R/abstract)<br>\n<br>\nModels are named as MASS_ZX.tar.gz, where MASS is the initial He core mass in solar mass units, and X is the metallicity of the models. H-rich140.tar.gz contains the files for the H-rich model of Appendix B.<br>\n<br>\nEach tarball contains the history file, a few MESA profile saved at specific evolutionary phases (before turning on the hydro in MESA at each pulse and at the onset of core-collapse), and the file ejecta.data which contains the properties of the ejecta at the time they first become faster than the escape velocity. These can be used as input in CSM simulations. We also provide the input files to reproduce each model in the corresponding tarball, and template input files at mesastar.org.</p>", 
  "license": "https://creativecommons.org/licenses/by/4.0/legalcode", 
  "creator": [
    {
      "affiliation": "Flatiron Institute, CCA", 
      "@id": "https://orcid.org/0000-0002-6718-9472", 
      "@type": "Person", 
      "name": "Renzo, M."
    }, 
    {
      "affiliation": "University of Amsterdam, API", 
      "@id": "https://orcid.org/0000-0003-3441-7624", 
      "@type": "Person", 
      "name": "Farmer, R."
    }, 
    {
      "affiliation": "Chinese accademy of Science", 
      "@id": "https://orcid.org/0000-0001-7969-1569", 
      "@type": "Person", 
      "name": "Justham, S."
    }, 
    {
      "affiliation": "The observatories of the Carnegie institution", 
      "@id": "https://orcid.org/0000-0002-6960-6911", 
      "@type": "Person", 
      "name": "Gotberg, Y."
    }, 
    {
      "affiliation": "Harvard, CfA", 
      "@id": "https://orcid.org/0000-0001-9336-2825", 
      "@type": "Person", 
      "name": "de Mink,. S. E."
    }, 
    {
      "affiliation": "Geneva Observatory", 
      "@id": "https://orcid.org/0000-0002-7464-498X", 
      "@type": "Person", 
      "name": "Zapartas, E."
    }, 
    {
      "affiliation": "KU Leuven", 
      "@id": "https://orcid.org/0000-0002-0338-8181", 
      "@type": "Person", 
      "name": "Marchant, P."
    }, 
    {
      "affiliation": "Steward Observatory", 
      "@type": "Person", 
      "name": "Smith, N."
    }
  ], 
  "headline": "Predictions for the hydrogen-free ejecta of pulsational pair-instability supernovae", 
  "image": "https://zenodo.org/static/img/logos/zenodo-gradient-round.svg", 
  "datePublished": "2019-09-12", 
  "url": "https://zenodo.org/record/3406357", 
  "keywords": [
    "Massive stars", 
    "pulsational pair instability supernovae", 
    "circumstellar material", 
    "black holes"
  ], 
  "@context": "https://schema.org/", 
  "identifier": "https://doi.org/10.5281/zenodo.3406357", 
  "@id": "https://doi.org/10.5281/zenodo.3406357", 
  "@type": "ScholarlyArticle", 
  "name": "Predictions for the hydrogen-free ejecta of pulsational pair-instability supernovae"
}