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Visual Binary Stars: Data to Investigate Formation of Binaries
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
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Herbig Ae/Be Visual Binaries [PDF]
We present the results of a high-angular resolution spectro-imaging survey of a sample of isolated Herbig Ae-Be (HAeBe) stars aimed at searching for close companions. The fraction of wide binaries is found to be significantly higher in HAeBe stars than in solar-mass field dwarfs, and suggests a companion star fraction possibly larger than 1.
J. Bouvier, P. Corporon
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Orbits, masses and dynamical parallaxes of 12 visual binary systems [PDF]
In this paper the preliminary orbital elements are presented for the following double stars: WDS 00153+4412 = A 1256 AB, WDS 00470+2315 = HU 413, WDS 00520+3154 = A 924, WDS 01036+6341 = MLR 87, WDS 01131+2942 = A 1260, WDS 01158+0947 = A 2102, WDS 01200-
Olević Dragomir M.+3 more
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On the component masses of visual binaries
In the Sixth Catalog of Orbits of Visual Binary Stars we found those belonging to the Main Sequence to form a sample containing 432 visual binaries. Their total masses were obtained dynamically, i.e. they were calculated using the orbital elements and the new Hipparcos parallaxes.
Z. Cvetković, S. Ninković
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OMICRON CETI A VISUAL BINARY [PDF]
R. G. Aitken
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Two Visual Binary Orbits [PDF]
R. v. d. R. Woolley, L. S. T. Symms
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Parallaxes of four visual binaries.
Frederick Slocum
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The Angular Momentum in Visual Binaries [PDF]
O. J. Eggen
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We present a method to identify likely visual binaries in Gaia eDR3 that does not rely on parallax or proper motion. This method utilizes the various point-spread function sizes of Two Micron All Sky Survey (2MASS)/Gaia, where at
Ilija Medan, Sébastien Lépine
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Statistical study of visual binaries [PDF]
In this paper, some statistical distributions of wide pairs included in Double Star Catalogue are investigated. Frequency distributions and testing hypothesis are derived for some basic parameters of visual binaries. The results reached indicate that, it was found that the magnitude difference is distributed exponentially, which means that the majority
W. H. Elsanhoury+2 more
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