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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

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   +5 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

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
  +8 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

Orbits of Ten Visual Binary Stars [PDF]

open access: bronzeChinese Journal of Astronomy and Astrophysics, 2007
We present the orbits of ten visual binary stars: WDS 01015+6922, WDS 01424–0645, WDS 01461+6349, WDS 04374–0951, WDS 04478+5318, WDS 05255–0033, WDS 05491+6248, WDS 06404+4058, WDS 07479–1212, and WDS 18384+0850. We have also determined their masses, dynamical parallaxes and ephemerides.
Bojan Novaković
openalex   +3 more sources

Orbital elements of five close visual binary stars [PDF]

open access: greenAstronomische Nachrichten, 2000
Revised orbital elements of the visual binary stars STT 2, STT 4, BU 1015, STT 6 and BU 395 are given. Dynamical parallaxes and total masses of the systems have been calculated.
M. Scardia   +3 more
openalex   +5 more sources

Pairing function of visual binary stars [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACTAn all-sky sample of 1227 visual binaries based on Washington Double Star catalogue is constructed to infer the initial mass function (IMF), mass ratio, and projected distance distribution with a dedicated population synthesis model. Parallaxes from Gaia DR2 and Hipparcos are used to verify the distance distribution.
Dmitry Chulkov
openalex   +4 more sources

Visual Orbits of Wolf–Rayet Stars. I. The Orbit of the Dust-producing Wolf–Rayet Binary WR 137 Measured with the CHARA Array [PDF]

open access: goldThe Astrophysical Journal
Classical Wolf–Rayet (W-R) stars are the descendants of massive OB stars that have lost their hydrogen envelopes and are burning helium in their cores prior to exploding as Type Ib/c supernovae.
Noel D. Richardson   +21 more
doaj   +3 more sources

Classical Observations of Visual Binary and Multiple Stars [PDF]

open access: bronzeProceedings of the International Astronomical Union, 2006
AbstractChanges in the double star database are highlighted, describing various methods of observation (both historically and those of the past few years) and their effectiveness in different regimes of separation space. The various niches for wide- and narrow-field work as they apply to double and multiple stars are examined and the different types of
Brian D. Mason
openalex   +3 more sources

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