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Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C

Stefano Ciprini; Maurizio Busso


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{
  "DOI": "10.15161/oar.it/1446126848.58", 
  "abstract": "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.", 
  "author": [
    {
      "family": "Stefano Ciprini", 
      "given": ""
    }, 
    {
      "family": "Maurizio Busso", 
      "given": ""
    }
  ], 
  "id": "16766", 
  "issued": {
    "date-parts": [
      [
        2003, 
        11, 
        7
      ]
    ]
  }, 
  "language": "eng", 
  "publisher": "2003, MemSAIt-Suppl., vol.2, p. 233", 
  "title": "Mid-infrared photometry of carbon stars and perspectives for surveys in\n  the Magellanic Clouds from Dome-C", 
  "type": "chapter"
}
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