On the Proper Motions and Distribution of Flare Stars in the Pleiades

Details On the Proper Motions and Distribution of Flare Stars in the Pleiades On the Proper Motions and Distribution of Flare Stars in the Pleiades

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983afz....19..588m&link_type=abstract

Astrofizika, Vol.19, NO.3, P.588, 1983

Mathematics

Probability

6

Scientific paper

It has been shown that the surface and space densities of the Pleiades flare stars decrease with the increase of the distance from the aggregate centre not depending on the probability as to be or not to be a member of the aggregate computed by proper motions. The mean proper motions of flare stars increase with the distance from the aggregate centre.

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