Titlebook: Short-Period Binary Stars: Observations, Analyses, and Results; Eugene F. Milone,Denis A. Leahy,David W. Hobill Book 2008 Springer Science

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透明

Modeling the Hot Components in Cataclysmic Variables: Info on the White Dwarf and Hot Disk from GALEis visible and may be directly studied. Recent results from studies of this type have determined that pulsating white dwarfs in accreting systems exist in a different instability strip than single pulsators and that highly magnetic white dwarfs still have hot spots even when the mass transfer stream has ended.

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0067-0057 these objects are analyzed.Among the specific objects repor.Short-period binaries run the gamut from widely separated stars to black-hole pairs; in between are systems that include neutron stars and white dwarfs, and partially evolved systems such as tidally distorted and over-contact systems. Thes

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Gravitational Lensing in Compact Binary Systemsise due to time delays and magnification factors occurring as a result of gravitational lensing by other compact objects. The results are applied to the double pulsar PSR J0737-3039 to determine whether or not anomalous enhancements observed during the eclipse of pulsar A by pulsar B have the signat

Obstruction

Accreting Neutron Stars in Low-Mass X-Ray Binary Systemsnct types of high-frequency X-ray oscillations. These oscillations are powered by release of the binding energy of matter falling into the strong gravitational field of the star or by the sudden nuclear burning of matter that has accumulated in the outermost layers of the star. The frequencies of th

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