As a result of the cooperation between the Sofia Sky Archive Data Center (Bulgaria) and Bamberg Observatory (Germany), Royal Observatory of Edinburgh (UK), Konkoly Observatory (Hungary), Strasbourg Observatory, Institute of Astronomy in Cambridge (UK), etc., a programme for investigation of
the long-term behaviour of the Pleiades active dwarf stars (in particular, flare stars) is in progress. Existing plates in the Pleiades are found in different European plate archives, made since the end of the nineteenth century, by the searching tool of the wide-field plate database
(http://www.skyarchive.org), which provides detailed information for astronomical plate archives all over the world, as well as for plates themselves. We investigate the Pleiades flare stars (UV Cet-type stars) included in the flare Stars database and identified in the USNO A2.0 catalogue.
68 Pleiades plates are already digitized with different scanning machines such as PDS 1010 (Sofia), PDS 2020 (Münster), SUPER COSMOS (Edinburgh), APM (Cambridge), UMAX 3000 (Budapest) and Epson (Berlin).
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Astronomical databases and catalogues;
Open clusters and associations;
UV Cet-type stars
Document Type: Research Article
Bulgarian Academy of Sciences Institute of Astronomy 72 Tsarigradsko Shosse Boulevard 1784 Sofia Bulgaria
Royal Observatory Blackford Hill Edinburgh EH9 3H UK
Sofia University Faculty of Mathematics and Informatics 5 J. Bourchier Boulevard 1164 Sofia Bulgaria
Astrophysikalisches Institut Potsdam An der Sternwarte 16 D-14482 Potsdam Germany
Konkoly Observatory H-1525 Budapest Hungary
Observatoire Astronomique 11 rue de l'Universite 67000 Strasbourg France
Institute of Astronomy Madingley Road Cambridge CB3 0HA UK
Publication date: 2003-08-01
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