HD 66051, an eclipsing binary hosting a highly peculiar, HgMn-related star
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F17%3A00099899" target="_blank" >RIV/00216224:14310/17:00099899 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1038/s41598-017-05987-6" target="_blank" >http://dx.doi.org/10.1038/s41598-017-05987-6</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1038/s41598-017-05987-6" target="_blank" >10.1038/s41598-017-05987-6</a>
Alternative languages
Result language
angličtina
Original language name
HD 66051, an eclipsing binary hosting a highly peculiar, HgMn-related star
Original language description
HD 66051 is an eclipsing system with an orbital period of about 4.75 d that exhibits out-of-eclipse variability with the same period. New multicolour photometric observations confirm the longevity of the secondary variations, which we interpret as a signature of surface inhomogeneities on one of the components. Using archival and newly acquired high-resolution spectra, we have performed a detailed abundance analysis. The primary component is a slowly rotating late B-type star (T-eff = 12500 +/- 200 K; log g = 4.0, v sin i = 27 +/- 2 km s(-1)) with a highly peculiar composition reminiscent of the singular HgMn-related star HD 65949, which seems to be its closest analogue. Some light elements as He, C, Mg, Al are depleted, while Si and P are enhanced. Except for Ni, all the iron-group elements, as well as most of the heavy elements, and in particular the REE elements, are overabundant. The secondary component was estimated to be a slowly rotating A-type star (T-eff similar to 8000 K; log g = 4.0, v sin i similar to 18 km s(-1)). The unique configuration of HD 66051 opens up intriguing possibilities for future research, which might eventually and significantly contribute to the understanding of such diverse phenomena as atmospheric structure, mass transfer, magnetic fields, photometric variability and the origin of chemical anomalies observed in HgMn stars and related objects.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2017
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Scientific reports
ISSN
2045-2322
e-ISSN
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Volume of the periodical
7
Issue of the periodical within the volume
July
Country of publishing house
GB - UNITED KINGDOM
Number of pages
11
Pages from-to
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UT code for WoS article
000405895400003
EID of the result in the Scopus database
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