Titlebook: Neutron Stars and Their Birth Events; Wolfgang Kundt Book 1990 Kluwer Academic Publishers 1990 Accretion.Population.Supernova.accretion di

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Millisecond Pulsars: A New Population of Gamma Ray Sources?,y sources. These observations, in turn, have sparked renewed activity in trying to understand how pulsars work. The early attempts concentrated on the generation of the coherent radio radiation through which they were first detected. The energy in this radiation is, however, an extremely small fract

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Magnetic Field Decay In Cooling Neutron Stars, effects of the evolution of the neutron stars, which have not been previously taken into account, are included. The results confirm the earlier work of Sang and Chanmugam (1987) that the field does not decay exponentially as generally assumed, and that if it occupies the entire crust it decays by l

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,Thermal Field Growth In Neutron Stars: An Alternative To “Injection”?,rn spinning rather slowly, with periods in excess of 100 ms. In this note we examine whether a slow build-up of neutron star magnetic fields from very low initial values (~10. gauss) may provide a viable alternative to this, as has been suggested by some authors. We find that irrespective of whether

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The Origin and Evolution of X-ray Binaries and Low-Magnetic-Field Radio Pulsars,ls with massive X-ray binaries, low-mass X-ray binaries, and X-ray binaries in globular clusters, as well as the transformation of some of these into millisecond radio pulsars. The paper is tutorial, the emphasis is on simple semi-analytical description.

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,Lecture #5 — Quasi-Periodic Oscillations (QPO),illiseconds. This area of research attracted lots of attention in 1984 when intensity-dependent QPO were found in GX 5–1 in the frequency range ～20–35 Hz (Van der Klis et al. 1985). Since then, a lot of observational and theoretical work has been done. Various forms of QPO have been identified, and