Contamination of RR Lyrae stars from Binary Evolution Pulsators
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...
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| Опубліковано в: : | Advances in Astronomy and Space Physics |
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| Дата: | 2015 |
| Автор: | |
| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Головна астрономічна обсерваторія НАН України
2015
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| Онлайн доступ: | https://nasplib.isofts.kiev.ua/handle/123456789/119821 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Цитувати: | 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. |
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Digital Library of Periodicals of National Academy of Sciences of Ukraine| id |
nasplib_isofts_kiev_ua-123456789-119821 |
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Karczmarek, P. 2017-06-09T20:49:49Z 2017-06-09T20:49:49Z 2015 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. 2227-1481 DOI: 10.17721/2227-1481.5.24-28 https://nasplib.isofts.kiev.ua/handle/123456789/119821 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% 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. en Головна астрономічна обсерваторія НАН України Advances in Astronomy and Space Physics Contamination of RR Lyrae stars from Binary Evolution Pulsators Article published earlier |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
Contamination of RR Lyrae stars from Binary Evolution Pulsators |
| spellingShingle |
Contamination of RR Lyrae stars from Binary Evolution Pulsators Karczmarek, P. |
| title_short |
Contamination of RR Lyrae stars from Binary Evolution Pulsators |
| title_full |
Contamination of RR Lyrae stars from Binary Evolution Pulsators |
| title_fullStr |
Contamination of RR Lyrae stars from Binary Evolution Pulsators |
| title_full_unstemmed |
Contamination of RR Lyrae stars from Binary Evolution Pulsators |
| title_sort |
contamination of rr lyrae stars from binary evolution pulsators |
| author |
Karczmarek, P. |
| author_facet |
Karczmarek, P. |
| publishDate |
2015 |
| language |
English |
| container_title |
Advances in Astronomy and Space Physics |
| publisher |
Головна астрономічна обсерваторія НАН України |
| format |
Article |
| description |
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%
|
| issn |
2227-1481 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/119821 |
| citation_txt |
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. |
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2025-12-07T18:33:24Z |
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