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astro-ph2003
Mid-infrared photometry of carbon stars and perspectives for surveys in the Magellanic Clouds from Dome-C
Stefano Ciprini, Maurizio Busso
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 c…
astro-ph2003
Blazars: the next gamma-ray view of GLAST
Stefano Ciprini
Blazars, the extreme family of AGN, can be strong gamma-ray emitters and constitute the largest fraction of identified point sources of EGRET. The next Gamma-ray Large Area Space T…