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Accretion disks in interacting binary stars
Scientific American, 1992J. Cannizzo, R. Kaitchuck
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Neutron Stars in Interacting Binary Systems [PDF]
Annual Review of Astronomy and Astrophysics, 1984 The early history of the development of our understanding of neutron stars has been described by others, and we summarize it only briefly here. Following an early speculation by Baade & Zwicky ( 1934) soon after the discovery of the neutron in 1932, Oppenheimer & Volkoff(1939) presented a classic analysis of the theoretical viability of neutron stars ...
Saul Rappaport, Paul C. Joss
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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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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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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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Evolutionary Processes in Interacting Binary Stars
, 1992R. Polidan, Yoji Kondo, Roberto Slstero
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Dynamics of Close Binary Systems; Double Stars; and Interacting Binary Stars
, 1979Z. Kopal +4 more
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