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Long-term Speckle Interferometric Monitoring of Binary Systems:2007–2023Positional Measurements and Orbits of Seven Objects

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Research in Astronomy and Astrophysics 2024年第9期24卷 147-155页

作者： arina mitrofanova Vladimir Dyachenko Anatoly Beskakotov Yuri Balega Alexander Maksimov Denis Rastegaev Special Astrophysical Observatory 369167 Nizhnij ArkhyzRussia

The results of seventeen years of speckle interferometric monitoring of seven objects(Chara 122Aa,GJ 3010,HIP1987,GJ 3076,HIP 11253,HIP 11352,and HIP 14929)are *** data were obtained at the 6 m Big Telescope Alt-azimuthal Special Astrophysical Observatory of the Russian Academy of Science(BTA SAO RAS)from 2007 to the *** of previously published and new measurements made it possible to construct completely new orbits for Chara 122Aa,HIP 11253,and HIP *** orbit of GJ 3076 cannot be constructed accurately due to the large influence of the weights assigned to the *** resulting orbital solutions are classified based on a grading scheme suggested by ***,*** and ***;most orbits are“definitive”(Grade 1).The mass sums and masses of components calculated by two independent methods using Hipparcos and Gaia DR2 and DR3 parallaxes were compared for the objects under study.

关键词： techniques:high angular resolution (stars:)binaries:visual stars:fundamental parameters stars:low-mass stars:solar-type

The first results of observations of lunar occultations in different spectral ranges at the 6-m telescope of the SAO RAS

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Research in Astronomy and Astrophysics 2020年第11期20卷 231-234页

作者： Ekaterina Shmaylova Vladimir Dyachenko Andrea Richichi Anatoly Beskakotov AleksandrMaksimov arina mitrofanova Yuri Balega Special Astrophysical Observatory Russian Academy of SciencesNizhniy ArkhyzKarachai-Cherkessian RepublicRussia 369167 Astronomical Institute St.Petersburg State UniversityUniversitetskij Pr.28Petrodvorets198504St.PetersburgRussia INAF-Osservatorio Astrofisico di Arcetri Largo E.Fermi 550125FirenzeItaly

Observations by the method of lunar occultations at the 6-m telescope of the SAO RAS reach a resolution limit better than *** have devised a new method of observation,which allows obtaining the curves of lunar occultations simultaneously in different ranges of the visible part of the spectrum,and conducted the first observations using amodified optical *** January 2019,applying the newmethod,the magnitude differences of the components of the binary star HD 36524 in the R and I bands were measured,which were 1.5 and 1.3mag,respectively,in good agreement with values calculated from the Gaia *** to the obtained data,it was determined that with this method it is possible to reach a signal-to-noise ratio of about 5–10 for stars of 10th *** discuss the applicability of the proposed optical scheme for the study of binary stars.

关键词： star binaries general instrumentation high angular resolution methods observational

On the correctness of orbital solutions obtained from a small set of *** of HIP 53731

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Research in Astronomy and Astrophysics 2020年第11期20卷 321-324页

作者： arina mitrofanova Vladimir Dyachenko Anatoly Beskakotov Yury Balega Alexander Maksimov Denis Rastegaev Sergey Komarinsky Special Astrophysical Observatory of the Russian Academy of Sciences Nizhnij ArkhyzRussia 369167

HIP 53731 is a binary consisting of stars of the spectral types K0 and *** orbit of this object was constructed previously by Cvetkovic et *** improved by *** should be noted that there is a 180°ambiguity in the position angles of some published *** interferometric observations were obtained in 2007–2020(21 measurements)at the 6-m telescope of the SAO RAS(BTA)by the authors of this *** analysis of new data together with previously published ones made it possible to construct an accurate orbit of HIP 53731 and to halve the already known values of the orbital period of the *** a result of the study,the mass sum,the masses of each component and their spectral types were determined by two independent *** to the qualitative classification of orbits,the orbital solution has grade 2–"good"(observations cover more than half of the orbital period and correspond to different phases).

关键词： techniques high angular resolution,speckle interferometry stars low-mass,fundamental parameters stars binaries spectroscopic stars individual HIP 53731

Research on the HIP 18856 binary system

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Research in Astronomy and Astrophysics 2021年第3期21卷 69-72页

作者： Polina Efremova arina mitrofanova Vladimir Dyachenko Anatoly Beskakotov Alexander Maksimov Denis Rastegaev Yury BalegaSergey Komarinsky Kazan Federal University Kazan 420008Russia Special Astrophysical Observatory of the Russian Academy of Sciences Nizhnij ArkhyzRussia 369167

The results of a study on the binary HIP 18856 and construction of its orbit are *** observational data were obtained at the BTA of SAO RAS in ***,Cvetkovic et *** the orbit for this ***,it is based on six measurements,which cover a small part of the *** positional parameters of the ESA astrometric satellite Hipparcos published speckle interferometric data(Mason et al.,Balega et al.,Horch et al.)and new ones were used in this *** on the new orbital parameters,the mass sum was calculated and the physical parameters of the components were *** obtained orbital and fundamental parameters were compared with the data from the study by Cvetkovic et al..The comparison shows that the new orbital solution is better than the old one,since it fits new observational data *** based on a qualitative evaluation performed by Worley&Heintz,the new orbit was classified as"reliable",which means data cover more than half of the orbit with sufficient quantities of residuals of measurements.

关键词： techniques:high angular resolution,speckle interferometry stars:low-mass,fundamental parameters stars:binaries:spectroscopic stars:individual:HIP 18856