Statistics – Computation
Scientific paper
May 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985afz....22..531g&link_type=abstract
(Astrofizika, vol. 22, May-June 1985, p. 531-544) Astrophysics (ISSN 0571-7132), vol. 22, no. 3, Nov. 1985, p. 315-323. Translat
Statistics
Computation
3
Late Stars, Red Dwarf Stars, Spectral Energy Distribution, Statistical Analysis, Stellar Flares, Computational Astrophysics, Star Clusters, Stellar Luminosity, Stellar Magnitude, Stellar Physics
Scientific paper
Accounting the observed power character of the energy spectrum of flares of UV Cet-type stars, several statistical characteristics of these stars are considered. It is shown that the mean amplitude of flares is mainly determined with the amplitude of the faintest flare that can be registered at the star under consideration and therefore - contrary to tradition - the mean flare amplitude cannot be used as a measure of flare activity of the star. On the basis of the Catalogue of flare stars in the Pleiades by Haro, Chavira and Gonzalez (1982), the luminosity function of these stars is constructed. Using this function and the revealed dependence of flare mean frequencies on stellar absolute magnitudes, the distribution of flare stars in the Pleiades along flare mean frequencies is constructed.
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