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- W4240085216 abstract "Four flares were observed on the late-type binary YY Gem in March 1988 during a total monitoring time of 408 min. The flares were unusual in that there is a periodicity in their occurrence, being separated by 48 ± 3 min. Considering the flares to be formed as a stochastic process, we find that the probability of these events occurring by chance is 0.5%. Modelling indicates that for quite reasonable input parameters (e.g. a spot field strength of 1000 G and a filament with mass per unit length of 10 6 g cm -1 ), the flare periodicity can be explained in terms of filament oscillations. The only requirement is that there should be a filament at these heights where the magnetic field drops inversely proportional to the height." @default.
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- W4240085216 date "1990-01-01" @default.
- W4240085216 modified "2023-10-17" @default.
- W4240085216 title "A model for the observed periodicity in the flaring rate on YY Gem" @default.
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- W4240085216 doi "https://doi.org/10.1017/s0074180900187947" @default.
- W4240085216 hasPublicationYear "1990" @default.
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