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First detailed analysis of multiple system V2083 Cyg
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SYSNO ASEP 0388576 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title First detailed analysis of multiple system V2083 Cyg Author(s) Zasche, P. (CZ)
Svoboda, P. (CZ)
Šlechta, Miroslav (ASU-R) RID, ORCIDSource Title Monthly Notices of the Royal Astronomical Society. - : Oxford University Press - ISSN 0035-8711
Roč. 421, č. 2 (2012), s. 1196-1200Number of pages 5 s. Language eng - English Country GB - United Kingdom Keywords stars ; binaries ; fundamental parameters Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000302695600021 DOI 10.1111/j.1365-2966.2012.20381.x Annotation The main aim of this paper is the first detailed analysis of multiple system V2083 Cyg, to reveal its basic physical properties. The system was studied using the methods of light-curve and radial-velocity curve analysis, together with interferometric data from the visual pair obtained during the last century. It was found that the close subsystem contains two very similar stars of spectral type A7-8. Moreover, a third body is orbiting around this pair with a period of about 177 yr. Due to the discrepancy in the total mass derived with the two methods, the possibility arises that the third body is perhaps also a binary, or some object with lower luminosity but higher mass than a normal main-sequence star. Another explanation is that the Hipparcos value of parallax is incorrect and the system is much closer to the Sun. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2013
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