INFRARED PHOTOMETRY OF UV CETI STARS
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Observatorio Astrofísico de Tonantzintla, Pue, Pue, Mex
Abstract
Infrared photometry is performed on twenty seven M-type dwarf stars, of which nine are stars of the UV Ceti type. The purpose of this study has been to search for infrared excesses in the flare stars. The result of the observations indicates that these st