Titlebook: Neutron Stars and Pulsars; Werner Becker Book 2009 Springer-Verlag Berlin Heidelberg 2009 Gravitational Waves from Spinning Neutron Stars.

AUGER

Rotating Radio Transients,uch as gamma-ray bursts, soft gamma-ray repeaters and anomalous X-ray pulsars. The situation at radio wavelengths, however, is dramatically different. While radio telescopes typically have sensitivity to events with short timescales, they have much narrower fields of view than their high-energy coun

Charade

Intermittent Pulsars,ently discovered types of transient radio source, namely the Rotating Radio Transient sources (RRATs) and the Intermittent Pulsars. Both spend much of their time invisible in quite different ways, and both have underlying periodicities which are attributable to rotating magnetic neutron stars. In th

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搖曳

Millisecond Pulsars in Globular Clusters and the Field, Galaxy at large. X-ray observations of globulars with imaging grazing incidence telescopes have proven to be at least as sensitive as radio telescopes for MSP detection and spectral classification, but not (yet) for period discovery due to the relatively low count rates. However, for known periods,

諷刺滑稽戲劇

Theory of Radiative Transfer in Neutron Star Atmospheres and Its Applications,sources of thermal X-ray emission, having surface temperatures of about one million Kelvin [11, 78]. This prediction and the discovery of the first pulsar became one of many motivations for further developing X-ray astronomy at the end of the 1950s. Observational study of thermal radiation from neut

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Neutron Star Cooling: I,isolated neutron stars. Results of numerical calculations,. for both minimal and enhanced cooling scenarios, are presented and compared with observational data..The first conjectures about the possible existence of stellar neutron cores by Landau [37] and Baade and Zwicky [6] and the pioneering work

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