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Titlebook: Isolated Neutron Stars: From the Surface to the Interior; Silvia Zane,Roberto Turolla,Dany Page Conference proceedings 2007 Springer Scien

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书目名称Isolated Neutron Stars: From the Surface to the Interior
编辑Silvia Zane,Roberto Turolla,Dany Page
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图书封面Titlebook: Isolated Neutron Stars: From the Surface to the Interior;  Silvia Zane,Roberto Turolla,Dany Page Conference proceedings 2007 Springer Scien
描述.This book collects the contributions presented at the conference .Isolated Neutron Stars: From the Surface to the Interior, .held in London in April 2006. Forty years after the discovery of radio pulsars it presents an up-to-date description of the new vision of isolated neutron stars that has emerged in recent years with the advance of multi-wavelength observations. The great variety of isolated neutron stars, from pulsars to magnetars, some of them discovered very recently and many of them not detectable in radio wavelengths, is amply covered by descriptions of recent observational results and presentations of the latest theoretical interpretation of these data..
出版日期Conference proceedings 2007
关键词Accretion; Corona; Plasma; cyclotron; equation of state; gravitation; magnetosphere; neutron; neutron star; s
版次1
doihttps://doi.org/10.1007/978-1-4020-5998-8
isbn_ebook978-1-4020-5998-8
copyrightSpringer Science+Business Media B.V. 2007
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,The continuum and line spectra of SGR 1806-20 bursts, feature. We examined whether theses spectral lines are dependent upon the choice of a particular continuum model and find no such dependence. Besides, we find that the 5 keV feature is pronounced with high confidence in the cumulative joint spectrum of the entire burst sample, both in the individua
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,The anatomy of a magnetar: XMM monitoring of the transient anomalous X-ray pulsar XTE J1810–197,s now consistent with the previous lack of detected pulsations in quiescence. We also summarize the detections of radio emission from XTE J1810–197, the first confirmed for any AXP. We consider possible models for the emission geometry and mechanisms of XTE J1810–197.
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,PSR J1119–6127 and the X-ray emission from high magnetic field radio pulsars,e emission has been found in high-magnetic-field radio pulsars, the X-ray characteristics of PSR J1119–6127 require alternate models from those of conventional thermal emission from neutron stars. In addition, PSR J1119–6127 is now the radio pulsar with the smallest characteristic age from which the
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