Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C
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 sma...
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ftdatacite:10.15161/oar.it/1446126848.58 2023-05-15T13:36:22+02:00 Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C Ciprini, Stefano Busso, Maurizio 2003 https://dx.doi.org/10.15161/oar.it/1446126848.58 https://www.openaccessrepository.it/record/16766?ln=en en eng 2003, MemSAIt-Suppl., vol.2, p. 233 Text ScholarlyArticle article-journal Publication 2003 ftdatacite https://doi.org/10.15161/oar.it/1446126848.58 2021-11-05T12:55:41Z 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. Text Antarc* Antarctic DataCite Metadata Store (German National Library of Science and Technology) Antarctic The Antarctic |
institution |
Open Polar |
collection |
DataCite Metadata Store (German National Library of Science and Technology) |
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ftdatacite |
language |
English |
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. |
format |
Text |
author |
Ciprini, Stefano Busso, Maurizio |
spellingShingle |
Ciprini, Stefano Busso, Maurizio Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C |
author_facet |
Ciprini, Stefano Busso, Maurizio |
author_sort |
Ciprini, Stefano |
title |
Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C |
title_short |
Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C |
title_full |
Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C |
title_fullStr |
Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C |
title_full_unstemmed |
Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C |
title_sort |
mid-infrared photometry of carbon stars and perspectives for surveys in the magellanic clouds from dome-c |
publisher |
2003, MemSAIt-Suppl., vol.2, p. 233 |
publishDate |
2003 |
url |
https://dx.doi.org/10.15161/oar.it/1446126848.58 https://www.openaccessrepository.it/record/16766?ln=en |
geographic |
Antarctic The Antarctic |
geographic_facet |
Antarctic The Antarctic |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_doi |
https://doi.org/10.15161/oar.it/1446126848.58 |
_version_ |
1766077670300319744 |