November 7, 2003 Book section Open Access

Stefano Ciprini; Maurizio Busso

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  <dc:creator>Stefano Ciprini</dc:creator>
  <dc:creator>Maurizio Busso</dc:creator>
  <dc:date>2003-11-07</dc:date>
  <dc:description>A preliminary analysis of the data from the MSX space infrared satellite,
seems to confirm that the [8.8]-[12.5] micron color index is well correlated
with the mass-loss rates in carbon stars of our Galaxy. The extension of this
mid-infrared observation criterion to the Magellanic Clouds, with a small-size
telescope, able to perform a continuous survey from Dome-C on the Antarctic
Plateau, could be crucial to trace the local AGB population and evolution.</dc:description>
  <dc:identifier>https://www.openaccessrepository.it/record/16766</dc:identifier>
  <dc:identifier>10.15161/oar.it/1446126848.58</dc:identifier>
  <dc:language>eng</dc:language>
  <dc:publisher>2003, MemSAIt-Suppl., vol.2, p. 233</dc:publisher>
  <dc:relation>info:eu-repo/semantics/altIdentifier/arxiv/arXiv:0308378v2</dc:relation>
  <dc:relation>url:https://www.openaccessrepository.it/communities/infn</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by-nc-nd/4.0/</dc:rights>
  <dc:title>Mid-infrared photometry of carbon stars and perspectives for surveys in
  the Magellanic Clouds from Dome-C</dc:title>
  <dc:type>info:eu-repo/semantics/bookPart</dc:type>
  <dc:type>publication-section</dc:type>
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