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Explaining the luminosity spread in young clusters: proto and pre-main sequence stellar evolution in a molecular cloud environment

Jensen, Sigurd S.; Haugbølle, Troels


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{
  "description": "<p>MESA inlists associated with <a href=\"https://ui.adsabs.harvard.edu/?#abs/2018MNRAS.474.1176J\">Jensen &amp;&nbsp;Haugb&oslash;lle (2018)</a>. MESA version 8845.</p>\n\n<p>Publication DOI:&nbsp;<a href=\"https://doi.org/10.1093/mnras/stx2844\">10.1093/mnras/stx2844</a></p>", 
  "license": "https://creativecommons.org/licenses/by/4.0/legalcode", 
  "creator": [
    {
      "@type": "Person", 
      "name": "Jensen, Sigurd S."
    }, 
    {
      "@type": "Person", 
      "name": "Haugb\u00f8lle, Troels"
    }
  ], 
  "url": "https://zenodo.org/record/2595676", 
  "datePublished": "2019-03-16", 
  "version": "8845", 
  "@context": "https://schema.org/", 
  "distribution": [
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  "identifier": "https://doi.org/10.5281/zenodo.2595676", 
  "@id": "https://doi.org/10.5281/zenodo.2595676", 
  "@type": "Dataset", 
  "name": "Explaining the luminosity spread in young clusters: proto and pre-main sequence stellar evolution in a molecular cloud environment"
}
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