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The Red Dwarf Stars of the UV Ceti-Type in the Neighbourhood of the Sun

Published online by Cambridge University Press:  12 April 2016

N. I. Shakhovskaya  and
E. Schöffel

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The intensive patrol observations of red dwarf stars during last years, carried out in the Crimea, Chile, Catania, South Africa, Armenia, Japan and other observatories led to appreciable increase of number of known UV Ceti-type objects. It permits us to complete the known lists of the variables (1—4). At the same time it is worth-while to define more precisely the criteria to consider a star as the UV Ceti-type variable, and to carry out strong selection of the certain UV Cet-type variables from the objects suspected to be this type variables.

Type
II. Flare Stars: Recent Campaigns and New Insights
Information
International Astronomical Union Colloquium , Volume 15: New Directions and Frontiers in Variable Stars Research , 1971 , pp. 138 - 143
Copyright
Copyright © Cambridge University Press 1971

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