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:unknown
Published: arXiv 2003
Subjects:
Astrophysics astro-ph
FOS Physical sciences
Antarctic
The Antarctic
Concordia Station
Antarc*
Online Access:https://dx.doi.org/10.48550/arxiv.astro-ph/0308378
https://arxiv.org/abs/astro-ph/0308378
id ftdatacite:10.48550/arxiv.astro-ph/0308378
record_format openpolar
spelling ftdatacite:10.48550/arxiv.astro-ph/0308378 2023-05-15T13:55:57+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/10.48550/arxiv.astro-ph/0308378 https://arxiv.org/abs/astro-ph/0308378 unknown arXiv Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2003 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0308378 2022-04-01T16:36:44Z 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. : 5 pages, 3 figures. In: Memorie SAIt - Supplementi, 2003, vol. 2, "The scientific outlook for Astronomy and Astrophysics Research at the Concordia Station: Recommendations for Future Developments.", E.Fossat & M. Candidi editors. Proceed. of the International Workshop held in Capri, April 28-30, 2003. pag. 233 Text Antarc* Antarctic DataCite Metadata Store (German National Library of Science and Technology) Antarctic The Antarctic Concordia Station ENVELOPE(123.333,123.333,-75.100,-75.100)
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Astrophysics astro-ph
FOS Physical sciences
spellingShingle Astrophysics astro-ph
FOS Physical sciences
Ciprini, Stefano
Busso, Maurizio
Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C
topic_facet Astrophysics astro-ph
FOS Physical sciences
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. : 5 pages, 3 figures. In: Memorie SAIt - Supplementi, 2003, vol. 2, "The scientific outlook for Astronomy and Astrophysics Research at the Concordia Station: Recommendations for Future Developments.", E.Fossat & M. Candidi editors. Proceed. of the International Workshop held in Capri, April 28-30, 2003. pag. 233
format Text
author Ciprini, Stefano
Busso, Maurizio
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 arXiv
publishDate 2003
url https://dx.doi.org/10.48550/arxiv.astro-ph/0308378
https://arxiv.org/abs/astro-ph/0308378
long_lat ENVELOPE(123.333,123.333,-75.100,-75.100)
geographic Antarctic
The Antarctic
Concordia Station
geographic_facet Antarctic
The Antarctic
Concordia Station
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_rights Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004
http://arxiv.org/licenses/assumed-1991-2003/
op_doi https://doi.org/10.48550/arxiv.astro-ph/0308378
_version_ 1766262955599462400

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