Accretion Onto Magnetic Degenerate Stars

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Deposition, Magnetic Stars, Degenerate Matter, Neutron Stars, X Ray Binaries, Cataclysmic Variables, Finite Difference Theory, Hydrodynamics, Simulation, Stellar Magnetic Fields, Mass Transfer

Scientific paper

While the original objectives of this research program included the study of radiative processes in cataclysmic variables and the evolution of neutron star magnetic fields, the scope of the reported research expanded to other related topics as this project developed. This final report therefore describes the results of our research in the following areas: 1) Irradiation-driven mass transfer cycles in cataclysmic variables and low-mass X-ray binaries; 2) Propeller effect and magnetic field decay in isolated old neutron stars; 3) Decay of surface magnetic fields in accreting neutron stars and pulsars; 4) Finite-Difference Hydrodynamic simulations of mass transfer in binary stars.

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