HD 165246: an early-type binary with a low mass ratio
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F13%3A10174137" target="_blank" >RIV/00216208:11320/13:10174137 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201220388" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201220388</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201220388" target="_blank" >10.1051/0004-6361/201220388</a>
Alternative languages
Result language
angličtina
Original language name
HD 165246: an early-type binary with a low mass ratio
Original language description
Analyses of 13 FEROS spectra from the ESO archive and 617 V-band photometric observations from the ASAS3 database allowed us to demonstrate that HD 165246 is a double-lined spectroscopic binary. As an earlier finding revealed, HD 165246 is also an eclipsing system. We were able to derive consistent orbital and light-curve solutions and all basic physical properties of the system. The period of this O8V + B7V binary is 4(d).592706 and the semiamplitudes of the radial-velocity curves are K-1 = 55.5 km s(-1) and K-2 = 321 km s(-1). As the mass ratio is small (0.173), the secondary lines cannot be seen directly in the spectra; however the application of spectral disentangling allowed us to detect weak Balmer and He I lines of the secondary component. The primary component rotates with a high projected velocity of v sin i = 243 km s(-1). A combined radial-velocity and light-curve solution led to the component masses and radii expected for the young stars of the given spectral types. Due to
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/GAP209%2F10%2F0715" target="_blank" >GAP209/10/0715: Accurate physical properties of hot stars based on binary and multiple star studies</a><br>
Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2013
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astronomy and Astrophysics
ISSN
0004-6361
e-ISSN
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Volume of the periodical
550
Issue of the periodical within the volume
únor
Country of publishing house
FR - FRANCE
Number of pages
7
Pages from-to
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UT code for WoS article
000314879700002
EID of the result in the Scopus database
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