November 7, 2003 Book section Open Access

Stefano Ciprini; Maurizio Busso

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  "doi": "10.15161/oar.it/1446126848.58", 
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    "alternate_identifiers": [
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    "creators": [
      {
        "affiliation": "Physics Dept. & Astronomical Obs., University of Perugia", 
        "name": "Stefano Ciprini"
      }, 
      {
        "affiliation": "Physics Dept. & Astronomical Obs., University of Perugia", 
        "name": "Maurizio Busso"
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    ], 
    "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.", 
    "doi": "10.15161/oar.it/1446126848.58", 
    "imprint": {
      "publisher": "2003, MemSAIt-Suppl., vol.2, p. 233"
    }, 
    "language": "eng", 
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      "id": "cc-by-nc-nd-4.0"
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    "publication_date": "2003-11-07", 
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      "title": "Book section", 
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    "title": "Mid-infrared photometry of carbon stars and perspectives for surveys in\n  the Magellanic Clouds from Dome-C"
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  "revision": 4, 
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