A NEW SLOWFLARE STAR IN ORION
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UNAM, Instituto de Astronomía, CD MEXICO, DF, MEX
Observatorio Astrofísico de Tonantzintla, Pue, Pue, Mex
Observatorio Astrofísico de Tonantzintla, Pue, Pue, Mex
Abstract
Photometric and spectroscopic characteristics are defined of the "slow" and "fast" flare stars. A new case of a "slow" flare star in Orion, is presented. It showed an increase of > 8.4 magnitudes in UV, during a period of 118 minutes. The peculiar physica