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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Main Authors: Ciprini, Stefano, Busso, Maurizio
Format: Text
Language:English
Published: 2003, MemSAIt-Suppl., vol.2, p. 233 2003
Subjects:
Online Access:https://dx.doi.org/10.15161/oar.it/1446126848.58
https://www.openaccessrepository.it/record/16766?ln=en
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spelling 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)
op_collection_id 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
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