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2000MNRAS.319.1147T - Mon. Not. R. Astron. Soc., 319, 1147-1153 (2000/December-3)
ROSAT All-Sky Survey X-ray and EUV observations of YY Gem and AU Mic.
TSIKOUDI V. and KELLETT B.J.
Abstract (from CDS):
The {formmu4} ratio for both stars is at the `saturation' limit found in rapidly rotating dwarfs and the most active RS CVn stars. We suggest that the gradually varying components are the result of a period of continuous, unresolved flaring activity. Alternatively, they may be the result of the emergence and subsequent decay of a new magnetic active region on the stellar surface of these stars.
Abstract Copyright: 2000, Royal Astronomical Society
Journal keyword(s): stars: activity - stars: flare - stars: individual: YY Gem - stars: individual: AU Mic - stars: late-type
Simbad objects: 5
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