Subsystems of Flare Stars of Different Ages in Orion and the Pleiades

Details Subsystems of Flare Stars of Different Ages in Orion and the Pleiades Subsystems of Flare Stars of Different Ages in Orion and the Pleiades

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap.....37...36m&link_type=abstract

Astrophysics, Vol. 37, NO. 1/SEP, P. 36, 1994

Astronomy and Astrophysics

Astrophysics

Scientific paper

The two best-studied subsystems of flare stars, in Orion and the Pleiades, which are of considerably different ages, are compared. It is shown that the observed differences between them are consistent with the evolutionary status of flare stars that represent a stage in the evolution of red dwarfs. It is found that less luminous stars exhibit higher flare frequencies. For equally luminous stars, flare activity is lower in older stars.

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