Abstract
An investigation of the two-dimensional distribution of flare stars in the Pleiades led to the discovery of a dip in their surface density at a distance of 3.2 pc from the center of the cluster. The same feature is found in the three-dimensional distribution of these stars.
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Translated from Astrofizika, Vol. 42, No. 4, pp. 537–540, October–December, 1999.
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Chavushian, H.S., Oskanian, A.V. & Broutian, G.H. One new property of the distribution of flare stars in the Pleiades cluster. Astrophysics 42, 404–407 (1999). https://doi.org/10.1007/BF02700947
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DOI: https://doi.org/10.1007/BF02700947