Other
Scientific paper
Jun 1971
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971bott....6...39g&link_type=abstract
Boletín de los Observatorios de Tonantzintla y Tacubaya Vol. 6, pp. 39-46 (1971) (http://www.astroscu.unam.mx/~bott/)
Other
4
Stars: Activity, Stars: Variables: Other (Uv Ceti)
Scientific paper
As a result of the analysis of more than 900 recorded flare-ups of flare stars in the solar vicinity it is shown that: i) The frequency of flares, f, increases with decreasing absolute luminosity of the flare stars. For all stars the condition f_U > f_B > f_V is satisfied. ii) The mean flare amplitude is larger for lower absolute luminosities. iii) Although the distribution function of flare amplitudes, F(δ_m), varies for each flare star; in general, the relative amount of flare-ups of large amplitudes decreases with increasing absolute luminosity. iv) The energy radiated by the star during flare-up, E_f, is larger for intrinsically brighter stars. v) The relative amount of radiative energy released by the star during a flare-up, E_f/E^*, increases for lower absolute luminosity.
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