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dc.contributor.author Karczmarek, P.
dc.date.accessioned 2017-06-09T20:49:49Z
dc.date.available 2017-06-09T20:49:49Z
dc.date.issued 2015
dc.identifier.citation Contamination of RR Lyrae stars from Binary Evolution Pulsators / P. Karczmarek // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 1. — С. 24-28. — Бібліогр.: 7 назв. — англ. uk_UA
dc.identifier.issn 2227-1481
dc.identifier.other DOI: 10.17721/2227-1481.5.24-28
dc.identifier.uri http://dspace.nbuv.gov.ua/handle/123456789/119821
dc.description.abstract A Binary Evolution Pulsator (BEP) is a low-mass (0.26Mꙩ ) member of a binary system, which pulsates as a result of a former mass transfer to its companion. The BEP mimics RR Lyrae-type pulsations, but has completely different internal structure and evolution history. Although there is only one known BEP (OGLE-BLG-RRLYR-02792), it has been estimated that approximately 0.2% of objects classified as RR Lyrae stars can be undetected Binary Evolution Pulsators. In the present work, this contamination value is re-evaluated using the population synthesis method. The output falls inside a range of values dependent on tuning the parameters in the StarTrack code, and varies from 0.06% to 0.43% uk_UA
dc.description.sponsorship It is a pleasure to thank G. Pietrzy«ski for substantive guidance to this project. I am gratefull to K. Belczynski for sharing the StarTrack code and for many useful and valuable instructions. This research is supported by the Polish National Science Centre grant PRELUDIUM 2012/07/N/ST9/04246. uk_UA
dc.language.iso en uk_UA
dc.publisher Головна астрономічна обсерваторія НАН України uk_UA
dc.relation.ispartof Advances in Astronomy and Space Physics
dc.title Contamination of RR Lyrae stars from Binary Evolution Pulsators uk_UA
dc.type Article uk_UA
dc.status published earlier uk_UA


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