Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002pobeo..73...81b&link_type=abstract
Publications of the Astronomical Observatory of Belgrade (ISSN 0373-3742), No. 73, p. 81 - 90 (2002). In: Proceedings of the Thi
Astronomy and Astrophysics
Astronomy
1
Pleiades, Active Dwarfs, Periodicities, Photographic Sky Surveys
Scientific paper
A program for searching for long-term periodicity of the Pleiades active dwarf stars is presented. As a basis the Pleiades flare stars (or UV Cet type stars) from the Flare Stars Database, which are identified in the USNO A2.0 catalogue are used. The investigation for long-term variability will be made by the usage of European astronomical plate archives, included in the Wide-Field Plate Database (http://www.skyarchive.org), whose time distribution covers more than 100 years. Among these plate archives are those of Rozhen Observatory (Bulgaria), Konkoly Observatory (Hungary), Byurakan (Armenia), Potsdam (Germany), Royal Observatory of Edinburgh (UK), Bamberg (Germany), etc. Limited number of the existing plates in the Pleiades region are already digitized with different scaning machines as PDS 1010 (Sofia), PDS 2020 (Muenster), SUPER COSMOS (Edinburgh) and some flatbed scanners.
Borisova Ana P.
Hambly Nigel
Kalaglarsky G. D.
Tsvetkov Milcho K.
Tsvetkova Katya P.
No associations
LandOfFree
Search for long-term periodicity in the Pleiades active dwarf stars from photographic sky surveys does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Search for long-term periodicity in the Pleiades active dwarf stars from photographic sky surveys, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Search for long-term periodicity in the Pleiades active dwarf stars from photographic sky surveys will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1664613