Results 261 to 270 of about 55,703 (289)

Interaction of binary stars with clusters

Astronomy Letters, 2008
The interaction of a wide (more than 1000 AU) binary field star with a star cluster is considered. We estimate the probabilities of the binary disruption and the capture of both the entire binary and one or two of its components as a function of the initial velocity of the binary star relative to the cluster.
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Interactive stars: Normal and compact stars in close binaries

AIP Conference Proceedings, 1990
The missions planned for the 1990’s will greatly expand our knowledge of close binary systems and the physical phenomena that can be studied in a member of a close binary, from stellar active regions to the highest density black hole candidates known.
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Cataclysmic Variables as Interacting Binary Stars

1985
The periodical literature on cataclysmic variables (CVs) and closely related topics has grown rapidly in recent years. In the Astrophysical Journal alone, the number of papers published on this subject in 1982 was about 80, the rate having doubled in three years. The other major journals taken together yield a similar annual total.
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Interacting binary stars: The stream-disk impact

AIP Conference Proceedings, 1998
The 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

2008
IUE 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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Interacting binary stars

Endeavour, 1985
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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.
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Accretion Disks in Interacting Binary Stars

Scientific American, 1992
John K. Cannizzo, Ronald H. Kaitchuck
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Interacting Binaries and Mass Loss in Hot Stars

1988
Studies 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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Holographic approach to compact stars and their binary mergers

Progress in Particle and Nuclear Physics, 2022
Carlos Hoyos Badajoz, Niko Jokela, Aleksi Vuorinen   +2 more
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