November 7, 2003 Book section Open Access

Stefano Ciprini; Maurizio Busso

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  <identifier identifierType="DOI">10.15161/oar.it/1446126848.58</identifier>
  <creators>
    <creator>
      <creatorName>Stefano Ciprini</creatorName>
      <affiliation>Physics Dept. &amp; Astronomical Obs., University of Perugia</affiliation>
    </creator>
    <creator>
      <creatorName>Maurizio Busso</creatorName>
      <affiliation>Physics Dept. &amp; Astronomical Obs., University of Perugia</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Mid-infrared photometry of carbon stars and perspectives for surveys in
  the Magellanic Clouds from Dome-C</title>
  </titles>
  <publisher>INFN Open Access Repository</publisher>
  <publicationYear>2003</publicationYear>
  <dates>
    <date dateType="Issued">2003-11-07</date>
  </dates>
  <language>en</language>
  <resourceType resourceTypeGeneral="Text">Book section</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="arxiv">arXiv:0308378v2</alternateIdentifier>
    <alternateIdentifier alternateIdentifierType="url">https://www.openaccessrepository.it/record/16766</alternateIdentifier>
  </alternateIdentifiers>
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  <rightsList>
    <rights rightsURI="https://creativecommons.org/licenses/by-nc-nd/4.0/">Creative Commons Attribution-NonCommercial-NoDerivatives</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">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.</description>
  </descriptions>
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