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Interacting binary stars: The stream-disk impact
AIP Conference Proceedings, 1998The interaction of a tidal stream with an accretion disk is reviewed with emphasis on numerical simulations. Beginning with crude 2D simulations showing the formation of an accretion disk in close binary systems, computational hydrodynamics have aided the study of Roche lobe overflow and the consequent stream/disk impact for the past 20 years.
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Spectra of interacting binary white dwarf stars
2008IUE spectra of 4 known Interacting Binary White Dwarf (IBWD) stars show spectra with no hydrogen, only helium and some traces of metals. From the continuum spectra it is possible to model a disk component and a hot central object.
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Supernovae from Single Stars and Interacting Binaries
There has been dramatic recent progress in our understanding of core-collapse supernovae. This, for the first time, has allowed us to connect supernova progenitors with their supernova explosions (if successful) and their remnants. Some of these predictions are currently testable with O4 LIGO observations.openaire +1 more source
Accretion Disks in Interacting Binary Stars
Scientific American, 1992John K. Cannizzo, Ronald H. Kaitchuck
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Interacting Binaries and Mass Loss in Hot Stars
1988Studies of the ultraviolet spectra of hot interacting binaries reveal methods that may represent important new tools for probing the physical conditions in the winds emanating from hot stars. Two systems, Mu Sagittarii and UW CMa are taken as examples of how these methods can be utilized to investigate the physics of mass loss in such objects.
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A reference map of the human binary protein interactome
Nature, 2020Katja Luck, Dae-Kyum Kim, Luke Lambourne
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