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Orbits of Binary Stars: from Visual Measures to Speckle Interferometry [PDF]

open access: goldThe Astronomical Journal
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.
Andrei Tokovinin
doaj   +7 more sources

Statistical Analysis of a Comprehensive List of Visual Binaries [PDF]

open access: yesOpen Astronomy, 2015
Visual binary stars are the most abundant class of observed binaries. The most comprehensive list of data on visual binaries compiled recently by cross-matching the largest catalogues of visual binaries allowed a statistical investigation of ...
Kovaleva D.   +4 more
doaj   +5 more sources

Visual binaries among high-mass stars - An adaptive optics survey of OB stars in the NGC 6611 cluster [PDF]

open access: bronze, 2001
We have searched for visual binaries with projected separations in the range 200-3000 AU (0.1"-1.5") among a sample of 96 stars in the massive young NGC 6611 cluster, 60 of them being subsequently identified as high probability cluster members of mainly OB spectral type.
Gaspard Duchêne   +3 more
arxiv   +8 more sources

Orbits Of Five Visual Binary Stars [PDF]

open access: greenBaltic Astron.16:435-442, 2007, 2007
We presented here the orbital parameters for five visual binary stars calculated by using the new method which we named Sector Grid Search. Orbital parameters were obtained for the following stars: WDS 00152+2722 = ADS 195, WDS 02202+2949 = ADS 1780, WDS 11550$-$5606 = HIP 58106, WDS 16256$-$2327 = ADS 10049 and WDS 16256$-$2327 = ADS 10045.
Bojan Novaković
arxiv   +5 more sources

Visual Binary Stars: Data to Investigate Formation of Binaries

open access: goldOpen Astronomy, 2016
Statistics of orbital parameters of binary stars as well as statistics of their physical characteristics bear traces of star formation history. However, statistical investigations of binaries are complicated by incomplete or missing observational data ...
Kovaleva D.   +3 more
doaj   +6 more sources

Spectroscopy of close visual binary components of the stable shell star 1 Del [PDF]

open access: yesA&A 587, A22 (2016), 2016
Stable shell stars are ideal objects for studying basic physical principles of the formation of disks in Be stars. If these stars have a close unresolved visual companion, its contribution toward the modelling of the disk cannot be overlooked, as is sometimes done.
Jiří Kubát   +4 more
arxiv   +7 more sources

Some Photometric Characteristics of Population II Orbital Visual Binary Stars [PDF]

open access: hybridOpen Astronomy, 2003
A MV ,B−V diagram for metal-deficient, kinematically selected thick disk and halo visual binary stars with known orbits is presented. The magnitude differences Δm between the components are analyzed.
Bartkevičius A., Gudas A.
doaj   +4 more sources

ON-SKY DEMONSTRATION OF A LINEAR BAND-LIMITED MASK WITH APPLICATION TO VISUAL BINARY STARS [PDF]

open access: greenThe Astrophysical Journal, 2010
We have designed and built the first band-limited coronagraphic mask used for ground-based high-contrast imaging observations. The mask resides in the focal plane of the near-infrared camera PHARO at the Palomar Hale telescope and receives a well-corrected beam from an extreme adaptive optics system.
Justin R. Crepp   +4 more
core   +10 more sources

Orbital elements of six visual binary stars [PDF]

open access: greenAstronomische Nachrichten, 2001
Revised orbital elements of the visual binary stars STT 515, BU 4 AB, STF 183 AB, A 207, STT 43 and A 2413 are given. Dynamical parallaxes and total masses of the systems have been calculated.
M. Scardia   +3 more
  +10 more sources

Visual binary stars with known orbits in Gaia EDR3 [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society, 2022
ABSTRACT A total of 3350 objects from the Sixth Catalog of Orbits of Visual Binary Stars (ORB6) are investigated to validate Gaia Early Data Release 3 (EDR3) parallaxes and provide mass estimates for the systems. We show that two-thirds of binaries with a separation of 0.2–0.5 arcsec are left without a parallax solution in EDR3.
Dmitry Chulkov, O. Yu. Malkov
openalex   +3 more sources

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