First detailed analysis of multiple system V2083 Cyg

0388576 - ASÚ 2013 RIV GB eng J - Článek v odborném periodiku
Zasche, P. - Svoboda, P. - Šlechta, Miroslav
First detailed analysis of multiple system V2083 Cyg.
Monthly Notices of the Royal Astronomical Society. Roč. 421, č. 2 (2012), s. 1196-1200. ISSN 0035-8711. E-ISSN 1365-2966
Výzkumný záměr: CEZ:AV0Z10030501
Klíčová slova: stars * binaries * fundamental parameters
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 5.521, rok: 2012

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.
Trvalý link: http://hdl.handle.net/11104/0217469