A superflare on an M dwarf produced an Halpha blue-wing enhancement indicating an erupting prominence with a projected bulk blueshift of about 228 km/s and a record mass ratio to its host star.
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An Extreme Stellar Prominence Eruption Observed by LAMOST Time-Domain Spectroscopy
A superflare on an M dwarf produced an Halpha blue-wing enhancement indicating an erupting prominence with a projected bulk blueshift of about 228 km/s and a record mass ratio to its host star.