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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 | 
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| dc.identifier.uri | 
http://dspace.nbuv.gov.ua/handle/123456789/119821 | 
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| 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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