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The Realm of Interacting Binary Stars
Astrophysics and Space Science Library, 1993exaly +2 more sources
Cataclysmic Variables as Interacting Binary Stars
1985The 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.
Richard A Wade
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Interaction of binary stars with clusters
Astronomy Letters, 2008The 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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Accretion Disks in Interacting Binary Stars
Scientific American, 1992John K. Cannizzo, Ronald H. Kaitchuck
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Interactive stars: Normal and compact stars in close binaries
AIP Conference Proceedings, 1990The 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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Star-Disc Interactions and Binary Formation
International Astronomical Union Colloquium, 1992By the time a binary arrives on the main sequence, its dynamics have essentially become those of a simple two-body system, so that its orbital parameters are constants of the motion thereafter. This statement of course needs to be modified under several circumstances, such as where tidal effects, mass exchange or interactions with field stars come into
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AGB stars in binaries and the common envelope interaction
Proceedings of the International Astronomical Union, 2018AbstractOne may argue that, today, proceedings articles are not useful. Results belong in refereed papers and even reviews are best in publications that are long enough to do justice to the topic reviewed. In this short review, reflecting a presentation that was given at the IAU343 symposium, Why Galaxies Care about AGB Stars, I have therefore ...
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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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