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The Stellar Angular Correlation: Clues to Wide Binary Star Properties
Publications of the Astronomical Society of the Pacific, 1993The 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
2015Detection 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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A wide-orbit giant planet in the high-mass b Centauri binary system
Nature, 2021Markus Janson +2 more
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Probing the interior physics of stars through asteroseismology
Reviews of Modern Physics, 2021Conny Aerts
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The Evolution of Compact Binary Star Systems
Living Reviews in Relativity, 2014Konstantin A Postnov
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Formation of the widest binary stars from dynamical unfolding of triple systems
Nature, 2012Bo Reipurth
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Mass Loss: Its Effect on the Evolution and Fate of High-Mass Stars
Annual Review of Astronomy and Astrophysics, 2014Nathan Smith
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