November 7, 2003 Book section Open Access

Stefano Ciprini; Maurizio Busso

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  "@id": "https://doi.org/10.15161/oar.it/1446126848.58", 
  "@type": "ScholarlyArticle", 
  "creator": [
    {
      "@type": "Person", 
      "affiliation": "Physics Dept. & Astronomical Obs., University of Perugia", 
      "name": "Stefano Ciprini"
    }, 
    {
      "@type": "Person", 
      "affiliation": "Physics Dept. & Astronomical Obs., University of Perugia", 
      "name": "Maurizio Busso"
    }
  ], 
  "datePublished": "2003-11-07", 
  "description": "A preliminary analysis of the data from the MSX space infrared satellite,\nseems to confirm that the [8.8]-[12.5] micron color index is well correlated\nwith the mass-loss rates in carbon stars of our Galaxy. The extension of this\nmid-infrared observation criterion to the Magellanic Clouds, with a small-size\ntelescope, able to perform a continuous survey from Dome-C on the Antarctic\nPlateau, could be crucial to trace the local AGB population and evolution.", 
  "headline": "Mid-infrared photometry of carbon stars and perspectives for surveys in\n  the Magellanic Clouds from Dome-C", 
  "identifier": "https://doi.org/10.15161/oar.it/1446126848.58", 
  "image": "https://zenodo.org/static/img/logos/zenodo-gradient-round.svg", 
  "inLanguage": {
    "@type": "Language", 
    "alternateName": "eng", 
    "name": "English"
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  "license": "https://creativecommons.org/licenses/by-nc-nd/4.0/", 
  "name": "Mid-infrared photometry of carbon stars and perspectives for surveys in\n  the Magellanic Clouds from Dome-C", 
  "sameAs": [
    "http://arxiv.org/abs/arXiv:0308378v2"
  ], 
  "url": "https://www.openaccessrepository.it/record/16766"
}