The fast-rotating single M4 dwarf V374 Peg is a well-known laboratory for studying intense stellar activity in a stable magnetic topology.
As an observable proxy for the stellar magnetic field, we studied the stability of the light curve, and thus the spot configuration. The
light curve suggests a spot configuration that is stable over about 16 years, confirming the previous indications of a very stable magnetic
field. Spectral data indicates flares and a complex CME with falling-back and re-ejected material, with a maximal projected velocity of
~675km/s.
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