Frequency Distribution Function of Stellar Flares for Faint Stars in the Pleiades Cluster

Details Frequency Distribution Function of Stellar Flares for Faint Stars in the Pleiades Cluster Frequency Distribution Function of Stellar Flares for Faint Stars in the Pleiades Cluster

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ap.....45...15p&link_type=abstract

Astrophysics (English translation of Astrofizika), v. 45, Issue 1, p. 15-19 (2002).

Astronomy and Astrophysics

Astrophysics

Scientific paper

It is shown that to derive the distribution function of the average
frequency of stellar flares in a case in which the number of flares
observed in an aggregatation is small, a chronology of third flares can
be used to confirm the chronology of first flares. A concrete solution
for faint stars of the Pleiades cluster is given.

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