{
  "id": "1509.02779",
  "version": "v1",
  "published": "2015-09-09T13:48:46.000Z",
  "updated": "2015-09-09T13:48:46.000Z",
  "title": "Synthetic clusters of massive stars to test stellar evolution models",
  "authors": [
    "Cyril Georgy",
    "Sylvia Ekström"
  ],
  "comment": "2 pages, 1 figure, to appear in the proceedings of the IAUS 316 held at the IAU General Assembly in Honolulu (2015)",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "During the last few years, the Geneva stellar evolution group has released new grids of stellar models, including the effect of rotation and with updated physical inputs (Ekstr\\\"om et al. 2012; Georgy et al. 2013a,b). To ease the comparison between the outputs of the stellar evolution computations and the observations, a dedicated tool was developed: the Syclist toolbox (Georgy et al. 2014). It allows to compute interpolated stellar models, isochrones, synthetic clusters, and to simulate the time-evolution of stellar populations.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2015-09-09T13:48:46.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "test stellar evolution models",
      "synthetic clusters",
      "massive stars",
      "stellar models",
      "geneva stellar evolution group"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 2,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}