On the statistics of flare stars

Details On the statistics of flare stars On the statistics of flare stars

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980afz....16...97m&link_type=abstract

(Astrofizika, vol. 16, Jan.-Mar. 1980, p. 97-106.) Astrophysics, vol. 16, no. 1, July 1980, p. 67-72. Translation.

Astronomy and Astrophysics

Astrophysics

6

Flare Stars, Star Distribution, Stellar Evolution, Pleiades Cluster, Stellar Luminosity, Stellar Magnitude, T Tauri Stars

Scientific paper

The distribution of flare stars with respect to their absolute magnitude in aggregates of different ages shows that the mean luminosity of the flare stars decreases upon transition to older aggregates. The dependence of the relative flare activity on the luminosity of the star is determined using the Pleiades aggregate data; the known stars of the system are divided into a group capable of having flares with amplitudes above a specified magnitude epsilon, and a group which is not capable of such flares. The ratio of the number of flare stars in the two groups decreases with the increasing value of the specified epsilon number.

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