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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Bibliographic Details
Main Authors: Ciprini, Stefano, Busso, Maurizio
Format: Text
Language:unknown
Published: arXiv 2003
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.astro-ph/0308378
https://arxiv.org/abs/astro-ph/0308378