Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C

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dc.creatorCiprini, Stefano
dc.creatorBusso, Maurizio
dc.date2003-08-21
dc.date2003-11-07
dc.date.accessioned2026-07-07T02:09:17Z
dc.date.available2026-07-07T02:09:17Z
dc.descriptionA 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.description5 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
dc.identifierhttps://arxiv.org/abs/astro-ph/0308378
dc.identifierhttp://arxiv.org/abs/astro-ph/0308378
dc.identifier2003, MemSAIt-Suppl., vol.2, p. 233
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6378
dc.subjectAstrophysics
dc.titleMid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C
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