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The Stellar Angular Correlation: Clues to Wide Binary Star Properties

Publications of the Astronomical Society of the Pacific, 1993
The angular distribution of stars brighter than visual magnitude 14 is analyzed for evidence of gravitationally bound systems with widely separated components. Binary stars with separations on the order of 0.1 parsec are interesting as probes of Galactic dynamics, disk dark matter, the Oort comet cloud, and the postulated solar companion star, Nemesis.
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Dense circumstellar nebulae in wide binary central stars

2015
Detection of close binary central stars with periods of less than a day is now well-tested and routinely possible via photometric monitoring. For wide binary central stars with periods of weeks to years detection techniques are still in their infancy. Radial velocity monitoring programs are yet to be applied to very large samples and the method suffers
Frew, DJ   +7 more
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Planetary System Disruption Within Wide Binary Star Systems

2011
Because they are so weakly bound, the orbits of wide binary stars evolve greatly under the influence of the Galactic tide and impulses from passing field stars. Most systems eventually pass through phases of high eccentricity, and this can have catastrophic consequences for the planets orbiting within these binary systems. During these eccentric phases,
Kaib, N. A.   +2 more
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The wide binary fraction of solar-type stars: emergence of metallicity dependence at a < 200 au

Monthly Notices of the Royal Astronomical Society: Letters, 2019
Kareem El-Badry   +2 more
exaly  

Wide binary companions to massive stars and their use in constraining natal kicks

Monthly Notices of the Royal Astronomical Society, 2019
Hagai Perets   +2 more
exaly  

Presupernova Evolution of Massive Single and Binary Stars

Annual Review of Astronomy and Astrophysics, 2012
Norbert Langer
exaly  

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