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dc.contributor.author |
Karczmarek, P. |
|
dc.date.accessioned |
2017-06-09T20:49:49Z |
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dc.date.available |
2017-06-09T20:49:49Z |
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dc.date.issued |
2015 |
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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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