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相关论文: New orbits based on speckle interferometry at SOAR

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Orbits of 44 close and fast visual binaries are computed using the latest speckle observations; 23 orbits are determined for the first time, the rest are revisions, some quite substantial. Six combined orbits use radial velocities. The…

太阳与恒星天体物理 · 物理学 2017-08-30 Andrei Tokovinin

We present results from Speckle inteferometric observations of fifteen visual binaries and one double-line spectroscopic binary, carried out with the HRCam Speckle camera of the SOAR 4.1 m telescope. These systems were observed as a part of…

太阳与恒星天体物理 · 物理学 2021-03-10 Rene A. Mendez , Ruben M. Claveria , Edgardo Costa

Results of speckle observations at the 4.1-m SOAR telescope in 2012 (158 measures of 121 systems, 27 non-resolutions) are reported. The aim is to follow fast orbital motion of recently discovered or neglected close binaries and sub-systems.…

太阳与恒星天体物理 · 物理学 2015-06-05 Andrei Tokovinin

Several nearby solar-type dwarfs with variable radial velocity were monitored to find their spectroscopic orbits. First orbital elements of 15 binaries (HIP 12144, 17895, 27970, 32329, 38636, 39072, 40479, 43004, 73700, 79234, 84696, 92140,…

太阳与恒星天体物理 · 物理学 2018-02-07 N. A. Gorynya , A. Tokovinin

The results of speckle interferometric observations at the SOAR telescope in 2014 are given. A total of 1641 observations were taken, yielding 1636 measurements of 1218 resolved binary and multiple stars and 577 non-resolutions of 441…

太阳与恒星天体物理 · 物理学 2015-08-06 Andrei Tokovinin , Brian D. Mason , William I. Hartkopf , Rene A. Mendez , Elliott P. Horch

The results of speckle interferometric observations at the 4.1 m Southern Astrophysical Research Telescope (SOAR) in 2018 are given, totaling 3097 measurements of 2427 resolved pairs with separations from 11 mas to 5.9" (median 0.15",…

太阳与恒星天体物理 · 物理学 2019-07-17 Andrei Tokovinin , Brian D. Mason , Rene A. Mendez , Elliott P. Horch , Cesar Briceno

We present orbital elements and mass sums for eighteen visual binary stars of spectral types B to K (five of which are new orbits) with periods ranging from 20 to more than 500 yr. For two double-line spectroscopic binaries with no previous…

太阳与恒星天体物理 · 物理学 2017-10-25 Rene A. Mendez , Ruben M. Claveria , Marcos E. Orchard , Jorge F. Silva

We observed stars with variable radial velocities to determine their spectroscopic orbits. Velocities of 132 targets taken over a time span reaching 30 years are presented. They were measured with the correlation radial velocity…

太阳与恒星天体物理 · 物理学 2019-06-12 J. Sperauskas , V. Deveikis , A. Tokovinin

The speckle interferometry program at the the 4.1 m Southern Astrophysical Research Telescope (SOAR), started in 2008, now accumulated over 30,300 individual observations of 12,700 distinct targets. Its main goal is to monitor orbital…

太阳与恒星天体物理 · 物理学 2022-07-27 Andrei Tokovinin , Brian D. Mason , Rene A. Mendez , Edgardo Costa

Spectroscopic orbits are computed for inner pairs in 9 hierarchical multiple systems (HIP 19639, 60845, 75663, 76816, 78163, 78416, 80448, 84789, and HD 105080) and for one simple binary HIP 61840. All subsystems are double-lined, and their…

太阳与恒星天体物理 · 物理学 2018-10-24 Andrei Tokovinin

Knowledge of the orbits of visual binary stars has always been one of the fundamentals of astronomy. Based historically on the visual measures, nowadays the orbits rely more (or exclusively) on the accurate speckle data. This prompts…

太阳与恒星天体物理 · 物理学 2024-08-23 Andrei Tokovinin

Several nearby solar-type dwarfs with variable radial velocity were monitored to find their spectroscopic orbits. Orbital elements of HIP 179, 1989, 2981, 5276, 6439, 11218, 21443, 96434 are determined, as well as tentative orbits for HIP…

太阳与恒星天体物理 · 物理学 2015-06-19 N. A. Gorynya , A. Tokovinin

The results of speckle interferometric observations at the 4.1 m Southern Astrophysical Research Telescope (SOAR) in 2019 are given, totaling 2555 measurements of 1972 resolved pairs with separations from 15 mas (median 0.21") and magnitude…

太阳与恒星天体物理 · 物理学 2021-01-11 Andrei Tokovinin , Brian D. Mason , Rene A. Mendez , Edgardo Costa , Elliott P. Horch

We present 1066 speckle measurements of M dwarf multiples observed over 2021-2024, all taken with HRCam on the Southern Astrophysical Research 4.1 m telescope. Among these, 900 observations resolve companions in 212 pairs, with separations…

太阳与恒星天体物理 · 物理学 2026-01-28 Eliot Halley Vrijmoet , Andrei Tokovinin , Todd J. Henry , Jennifer G. Winters , Wei-Chun Jao , Elliott Horch

We report the discovery of 24 spectroscopic binary companions to giant stars. We fully constrain the orbital solution for 6 of these systems. We cannot unambiguously derive the orbital elements for the remaining stars because the phase…

We report high resolution optical speckle observations of 336 M dwarfs which result in 113 measurements of relative position of 80 systems and 256 other stars with no indications of duplicity. These are the first measurements for two of the…

太阳与恒星天体物理 · 物理学 2018-05-16 Brian D. Mason , William I. Hartkopf , Korie N. Miles , John P. Subasavage , Deepak Raghavan , Todd J. Henry

In a well-aimed search based on the recently published Gaia~DR2 radial velocity data and performed with the robotic TIGRE telescope, we have discovered 19 bright ($m_V<7.66$~mag) spectroscopic binary stars. We present the radial velocity…

太阳与恒星天体物理 · 物理学 2020-10-07 Dennis Jack , Missael Alejandro Hernández Huerta , Klaus-Peter Schröder

Based on a direct combination of the Hipparcos data with astrometric ground-based observational catalogues having epochs between 1938 and 1999 the preliminary orbits and component masses are calculated for 6 binaries with no previous orbit…

太阳与恒星天体物理 · 物理学 2016-06-29 G. A. Gontcharov , O. V. Kiyaeva

Results of speckle interferometry observations at the 4.1 m SOuthern Astrophysical Research (SOAR) telescope obtained during 2024-2025 are presented. We present 5316 measurements of relative positions and magnitude differences in 3532 pairs…

太阳与恒星天体物理 · 物理学 2026-05-05 Andrei Tokovinin , Brian D. Mason , Rene A. Mendez , Edgardo Costa

We present an analysis of nine bright spectroscopic binaries (HD 1585, HD 6613, HD 12390, HD 39923, HD 55201, HD 147430, HD 195543, HD 202699, HD 221643), which have orbital periods of P > 500 days. These well-separated binaries are the…

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