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

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 soluti...

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Veröffentlicht in:Astrophysics 2002-01, Vol.45 (1), p.15-19
1. Verfasser: Parsamian, Elma S
Format: Artikel
Sprache:eng
Schlagworte:
Astrophysics
Frequency distribution
Stars & galaxies
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Zusammenfassung: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.[PUBLICATION ABSTRACT]
ISSN:0571-7256
1573-8191
DOI:10.1023/A:1015338408013