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

甜食

Intermittent Pulsars,for intervals of time measured in days or years, with longer intervals when there is no emission at all. In this paper, we discuss the phenomenon, the search for other instances, the implications for pulsar magnetospheric physics and the galactic population of such objects.

Licentious

The Double Pulsar: A Unique Lab for Relativistic Plasma Physics and Tests of General Relativity,eak-field regime, while deviations from GR may appear only in strong gravitational fields. It happens that nature provides us with an almost perfect laboratory to test the strong-field regime using binary radio pulsars.

咽下

Isolated Neutron Stars: The Challenge of Simplicity, discovered rotating radio transients and the magnetar candidates in particular..First hypothesised in the 1930s, neutron stars have been for more than 40 years a theoretician‘s dainty, until the discovery of the first radio pulsar [27]. Since then, neutron stars have been mostly detected at radio w

Albinism

Millisecond Pulsars in Globular Clusters and the Field,) and overall populations. Observations of several nearby field MSPs with ., with its temporal-spectral resolution, have given new measurements of the M/R (compactness) of neutron stars from precise measures of their soft X-ray pulse profiles as a function of energy. X-ray spectral-timing of MSPs ca

偶然

Theory of Radiative Transfer in Neutron Star Atmospheres and Its Applications,eppoSAX added important information on the pulsar emission in the harder band pass whereas EUVE and HST allowed to study neutron stars in the very soft 0.07—0.2 keV and optical/UV bands. More details on results from observations of neutron stars can be found in the Chaps. 6—8. New excellent observat

Ige326

Neutron Star Cooling: II,ollowed by the second such Galactic X-ray source detection, this time in the Crab supernova remnant [15]. It was immediately suggested by several theorists [19, 59, 66] that these strong X-ray sources might be neutron stars, because if these X-rays are blackbody radiation as expected, the radius of