RAPID VARIABLES IN THE ORION NEBULA
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UNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
Abstract
During a study of the Ha emission stars in and near the Orion nebula Haro found a good number of cases where the Haemission line or the continuum varies in intensity strongly suggesting a "Flare" star. As a continuation of this work we have found 7 new st