NEW FLARE STARS AND THE SAN LUIS POTOSIECTRUM RATE OF VARIATION RELATION
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UNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
Abstract
In this study we confirm that whenever there is a group of T Tauri stars, there is the possibility of finding, associated to them, rapid variables. We have thus found 7 new variables of the UV Ceti Type in the Taurus dark region. From the new data we can
