Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980afz....16..677p&link_type=abstract
(Astrofizika, vol. 16, Oct.-Dec. 1980, p. 677-685.) Astrophysics, vol. 16, no. 4, Apr. 1981, p. 391-395. Translation.
Astronomy and Astrophysics
Astrophysics
9
Frequency Distribution, Orion Constellation, Stellar Flares, Distribution Functions, Pleiades Cluster, Star Clusters, Stellar Luminosity, Temporal Distribution
Scientific paper
The temporal distributions of flare stars in the Orion association and the numbers of stars with different flare frequencies are determined by means of Ambartsumian's (1978) method, which uses the chronology of discovery of 'first' flares and the chronology of confirmations, i.e., the temporal distributions of 'repeated' flares. It is shown that flare stars with high flare frequency (not greater than 1000 hours) in the Pleiades are basically stars of low luminosity with M(U) not less than 13m. Two independent methods of determining the number of flare stars in the aggregates confirm that there are about 1.5 times more flare stars in the Orion association than in the Pleiades.
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