Physical parameters and dynamical properties of the multiple star o and |
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| Authors: | R Ya Zhuchkov E V Malogolovets O V Kiyaeva V V Orlov I F Bikmaev YuYu Balega D I Safina |
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| Institution: | 1.Kazan (Privolzhskii) Federal University,Kazan’,Russia;2.Special Astrophysical Observatory,Russian Academy of Sciences,Nizhnii Arkhyz, Karachaevo-Cherkesskaya Republic,Russia;3.Main (Pulkovo) Astronomical Observatory,Russian Academy of Sciences,St. Petersburg,Russia;4.V.V. Sobolev Astronomical Institute,St. Petersburg State University,St. Petersburg,Russia |
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| Abstract: | An analysis of the physical characteristics, orbital parameters, and dynamical stability of the multiple Be star HD 217675
(o And) is presented. Observations on the 6-m SAO and 1.5-m RTT telescopes are used to refine the orbital parameters of the
subsystems. The spectral types, absolute magnitudes, and masses of the components are estimated. The total mass of the system
is 18 ± 2 M
db. It is shown that the configuration of the system is 2 + 2, where one of the subsystems is a spectral binary with a period
of 33 d and the outer pair has a period of 117 yr. The parameters of the second inner subsystem are uncertain, making it difficult
to draw firm conclusions about the stability of this multiple star. |
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