Observational program for binary systems with varied periods

Details Observational program for binary systems with varied periods Observational program for binary systems with varied periods

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ysc..conf...82s&link_type=abstract

12th Young Scientists' Conference on Astronomy and Space Physics, held in Kyiv, Ukraine, April 19-23, 2005, Eds.: Simon, A.; Gol

Physics

Space Physics

Scientific paper

"An Atlas of O-C Diagrams of Eclipsing Binary Stars" by Kreiner et al. [1] was published at the end of past century. Stars were included in the "Atlas..." provided they satisfied 3 criteria: 1) at least 20 minima had been timed; 2) these minima spanned at least 2,500 cycles; 3) the 2,500 cycles represented no fewer than 40 years. 3851 binary systems were include in "Atlas...", but for some stars with long-term period variations first criteria was not fulfilled. We discuss the observational program for this stars and firs results which were obtained in Kalinenkov Astronomical Observatory.

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